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REVIEW 4 major objections 5 minor 199 references

The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry

T0 review · 4 major / 5 minor · reviewed 2026-08-05 · deepseek-v4-flash

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Pith's one-line read Most massive Galactic stars are pulsators, and photometric variability is nearly ubiquitous.

desk verdict Solid Northern census with real new binaries and a sharp point about RV thresholds, but the missing detection threshold and inconsistent RV counts need fixing before the headline fractions can be trusted. read the letter →

arxiv 2608.03383 v1 pith:LTBQFB4M submitted 2026-08-04 astro-ph.SR

K. Thomson-Paressant , D. M. Bowman , F. Nardini , L. J. A. Scott , J. Bodensteiner , T. Shenar , L. Mahy , G. Handler
show 11 more authors
N. Shitrit I. Arcavi M. Abdul-Masih S. Simon-Diaz P. Van Daele A. J. Kalita L. Dennis J. Henneco A. Tkachenko H. Sana H. Van Winckel
This is my paper
classification astro-ph.SR
keywords massivestarsOBasteroseismologypulsatingspectroscopicbinarieseclipsingTESSphotometryradialvelocities
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The reading

This paper combines multi-epoch HERMES spectroscopy with 2-minute TESS photometry for 873 Galactic O- and B-type stars to measure how common pulsation, binarity, and rotational modulation are together in one population. It claims that more than 93 percent of the sample shows photometric variability, 82 percent show pulsations, and at least 14 percent show evidence of binarity, with only 58 of 873 stars appearing photometrically constant. The result matters because it turns the older picture of massive stars as mostly quiet into one where variability is the norm, giving a statistical foundation for asteroseismic modelling and for testing stellar evolution prescriptions. It also shows that the standard 20 km/s radial-velocity threshold used to identify spectroscopic binaries in massive stars can misclassify high-amplitude pulsators as binaries, and argues that photometry should inform binarity studies of Galactic massive stars.

What carries the argument

The central instrument is the combined dataset: multi-epoch high-resolution HERMES spectra (cross-correlated to measure radial velocities and fit TLUSTY model grids for Teff, log g, and vsini) paired with 2-minute-cadence TESS light curves analysed with modified generalised Lomb-Scargle periodograms on a per-sector basis. Variability classification gives priority to the dominant type consistently seen across sectors, and binarity is assessed with two spectroscopic criteria: a statistical 4-$\sigma$ RV difference and an absolute $\Delta$ RV threshold of 20 km/s. The paper also constructs empirical pulsation-instability regions from the density of stars of each pulsator type in the spectroscopic HR

What would settle it

Re-analyse a sample of the classified pulsators and the 58 'constant' stars using two or more consecutive TESS sectors together with injection-recovery simulations. If the low-frequency peaks identified as SPB or SLF disappear or change between sectors, or if the 58 constant stars show variability at the 10-micromagnitude level over a longer baseline, the 82 percent and 93 percent fractions and the empirical instability-region boundaries would need revision.

Watch

Extended reading notes

Core claim

The paper demonstrates that the vast majority of massive Galactic stars are pulsators, with a diversity of pulsations allowing identification of beta Cep stars, slowly pulsating B-type (SPB) stars, and stochastic low-frequency (SLF) variability. Photometric variability among massive stars appears nearly ubiquitous: only 58 of the 873 stars show no significant variability at all. Using the 33rd and 66th percentile density contours in a spectroscopic Hertzsprung-Russell diagram, the paper maps empirical instability regions for the three pulsator types, finds that the observed pulsator locations broadly match theoretical instability strips, and concludes that convective boundary mixing is likel

Load-bearing premise

The headline 82 percent pulsator fraction rests on treating a significant coherent peak in a single 27-day TESS sector as a true pulsation signal, with no stated false-alarm threshold, so instrumental or rotational low-frequency peaks could shift stars between pulsator classes and move the empirical instability regions.

Editorial extensions

If this is right

  • If variability is nearly ubiquitous among massive Galactic stars, the 58 apparently constant stars are likely detection-limited, and longer or more precise light curves should reveal variability in many of them.
  • The empirical instability regions for beta Cep, SPB, and SLF variability provide a direct statistical benchmark for stellar evolution models, and imply that convective boundary mixing is mass dependent above about 15 solar masses.
  • The finding that pulsation-induced RV variability can exceed the 20 km/s binary threshold means published binary fractions for Galactic B-type stars based on spectroscopy alone may be overestimated, and photometric information should be used alongside RVs.
  • At least 12 of the 67 eclipsing binaries also show beta Cep or SPB pulsations, making them promising systems for combining eclipse geometry with asteroseismology.
  • The 148 stars with rotational modulation, including 39 that also pulsate, are candidate magnetic stars that merit spectropolarimetric follow-up and possible magneto-asteroseismic study.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • Editorial inference: Because most stars have only one 27-day TESS sector, the reported pulsator fraction is likely a lower bound; multi-sector data with frequency-resolved coherence tests would probably push the 82 percent higher and sharpen the SPB versus SLF boundary.
  • Editorial inference: The paper's threshold analysis suggests that population-level corrections for pulsation-induced RV jitter should be applied when combining spectroscopic binary fractions across different Galactic B-type samples, otherwise the inferred intrinsic binary fraction may be inflated.
  • Editorial inference: The 30 newly discovered eclipsing binaries, half with periods shorter than 3 days, provide a ready sample for tidal-asteroseismology tests of binary evolution, but firm conclusions will require orbital solutions from further epochs.
  • Editorial inference: If the SLF variability detected here is dominated by internal gravity waves, the empirical instability regions imply that the convective-core boundary and near-core mixing prescriptions in stellar models can be calibrated statistically from these photometric demographics alone.
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Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, and a circularity audit.

Referee Report

4 major / 5 minor

Summary. The manuscript presents a combined photometric and spectroscopic census of 873 Galactic O- and B-type stars, using 2-min cadence TESS light curves and multi-epoch HERMES spectra. The authors classify the dominant photometric variability as SPB, beta Cep, stochastic low-frequency (SLF), rotational modulation, or eclipsing binary, and they use radial-velocity measurements to identify candidate spectroscopic binaries. Headline results are that >93% of the sample is photometrically variable, 82% show pulsations, and at least 14% show evidence of binarity. The paper also derives empirical instability regions for the three pulsator classes and compares them with the theoretical tracks/instability strips of Burssens et al. (2020).

Significance. If the headline fractions and classifications are reliable, this is one of the largest homogeneous variability surveys of massive stars in the Northern hemisphere and a useful complement to the southern Burssens et al. (2020) sample. The public data products, the large sample size, the machine-learning continuum normalization, and the cross-check with Gaia ESP-HS are strengths. The empirical instability regions and the identification of 30 new eclipsing binaries are valuable for future asteroseismic and binary-evolution modelling. However, the statistical foundations of the central fractions need substantial clarification before the results can be used as quantitative benchmarks.

major comments (4)
  1. [Section 2.4, Section 3] The Lomb-Scargle analysis never states the detection threshold: no false-alarm probability, signal-to-noise criterion, or peak-selection rule is given. The text only says 'we use the same classification criteria as Burssens et al. (2020)' without reproducing or summarizing them. This is load-bearing because the 82% pulsator fraction and the separation of SPB, beta Cep, and SLF variability depend entirely on which periodogram peaks are deemed significant. The paper itself warns that frequencies below about 0.5 d^-1 'could be instrumental (e.g. imperfect detrending) or astrophysical', exactly the regime where SPB and SLF classifications are made. With most stars having a single 27-day sector, an unstated threshold could inflate or shift the pulsator fractions. Please state the threshold and provide a robustness test showing how the pulsator fraction and Fig. 5 contours change for a range o
  2. [Section 3, Section 4.3, Table 2, Fig. 6] The reported counts are mutually inconsistent. Section 3 lists 197 SPB stars, 251 beta Cep stars, and 268 SLF stars, summing to 716, which is then used as 82% of 873. Section 4.3 and Fig. 6 instead report 200 beta Cep stars, 116 SPB stars, and 167 SLF stars, and the text refers to 664 pulsating stars. If the 716 number is the sum over non-exclusive classifications (e.g., a star counted as both SPB and beta Cep), then dividing by 873 overstates the unique pulsator fraction. If the smaller numbers refer only to the subset with successful vsini fits, that needs to be stated explicitly. Please give unique-star counts for each class and for the union of all pulsators, and reconcile every number in the text and figures.
  3. [Section 5.2, Abstract] The 'grand total of 124 binary systems' is a sum over overlapping populations: 22 SB2 systems, 28 SBX-catalogue targets, 67 eclipsing binaries, and 51 stars satisfying both RV criteria, with acknowledged cross-membership (10 EBs meet both RV criteria, 6 EBs are SB2). This sum cannot be used directly to claim 'at least 14% show evidence of binarity' without computing the union of unique binary stars. In addition, the RV-variability count is inconsistent: Section 2.2.3 says 277 of 377 stars with two or more epochs are RV variables, while Section 3 says 353 of 873 stars (or 76% of 464) have RV variability. These numbers must be reconciled and the analysis repeated with a consistent denominator.
  4. [Section 3, Abstract] The headline fractions are quoted as point estimates without statistical uncertainties. Given the selection function (V<14, the HERMES follow-up subset, and the variable number of TESS sectors from one to several), the abstract's '>93%', '82%', and 'at least 14%' should be accompanied by binomial confidence intervals or an equivalent statement of statistical precision. Without this, it is difficult to compare the fractions with Burssens et al. (2020) or to assess whether differences are significant.
minor comments (5)
  1. [Section 4.3] The sentence 'About half of the 664 pulsating stars are identified as slow-to-moderate rotators' is inconsistent with the numbers given: 301 of 664 is 45%, and 301+134=435 is 65%. Please rephrase or correct.
  2. [Fig. 6] The vertical-axis label 'Nb T argets' contains a typographical error; it should read 'Nb Targets'.
  3. [Section 5.3.1] The statement that 'the number of non-pulsating binaries that satisfy both criteria is 1 per cent of the full sample' should give the absolute count and the denominator, since it is easy to confuse with the 82/377 binary fraction.
  4. [Fig. 5] The caption uses 'large fractions' and the text defines 33rd and 66th percentiles, but it is not stated how the density contours are calculated (e.g., kernel density estimation, binning, or percentile-in-mass/log L). Please make the method explicit.
  5. [Section 2.2.3] The distinction between 'RV variability' and 'binarity candidates' would be easier to follow if the two criteria and their outputs were presented in a small table, especially because the counts 277, 353, 51, and 82 appear in different places.

Circularity Check

0 steps flagged · score 0.0 of 10

No significant circularity; the census is an observational analysis, not a fitted prediction.

full rationale

The paper's central claims are empirical demographics derived from TESS photometry and HERMES spectroscopy, not from a derivation that reduces to its own inputs. Pulsator and binarity classifications are assigned using periodogram analysis and adopted RV criteria (e.g., Eq. 1 with a 4.0 threshold and Eq. 2 with C = 20 km/s), which are literature conventions rather than parameters fitted to the headline fractions. The empirical instability regions in Fig. 5 are percentile contours of the classified sample itself, i.e., summaries of the data, not predictions produced by fitting theory to data. The comparison to Burssens et al. (2020) uses their MESA evolutionary tracks and GYRE instability strips as an external benchmark; although authorship overlaps, those calculations were not derived from the present sample and the agreement is a genuine, falsifiable comparison. The paper explicitly acknowledges limitations of the adopted criteria and the ambiguity of the 20 km/s threshold. The absence of a stated false-alarm probability for the Lomb-Scargle periodograms is a measurement-reliability and reporting concern, not a circularity, because the detection threshold is not itself the quantity being predicted. No equation or claim in the paper defines the 82% pulsator fraction or the 93% variability fraction in terms of the same fitted parameters used to produce them. Therefore, no circular step is present.

Assumptions & free parameters 4 free parameters · 6 assumptions · 0 invented entities

The central statistics depend on several hand-chosen thresholds and fixed model assumptions. The 20 km/s and 4.0-sigma RV thresholds, and the 33rd/66th percentile contour choices, are adopted or chosen rather than derived from the data. The TLUSTY fitting fixes metallicity and microturbulence, which biases stellar parameters. No new physical entities are introduced.

free parameters (4)
  • RV binarity threshold C = 20 km/s
    Adopted from Sana et al. (2012, 2013) and used in Eq. 2 to classify spectroscopic binaries. The paper itself demonstrates this threshold is ambiguous for galactic B-type pulsators, and the binary catalog depends on it (51 stars pass both criteria).
  • RV significance threshold = 4.0
    Adopted threshold in Eq. 1 for statistically significant RV variability; affects the first binarity criterion.
  • Empirical instability region percentiles = 33rd and 66th percentiles
    Chosen to define the empirical instability regions in Fig. 5; these percentile levels determine the contour boundaries and are not derived from theory.
  • Microturbulence vmic for O-star grid = 10 km/s
    Fixed microturbulence in the TLUSTY O-star grid (Section 2.2.4); this choice affects stellar parameter determination and hence HR positions.
assumptions (6)
  • domain assumption The Lomb-Scargle periodogram significance threshold used to identify frequencies is appropriate
    Section 2.4 declares significant peaks without specifying the false-alarm probability or amplitude criterion; all pulsator classifications depend on this.
  • domain assumption TLUSTY grid with fixed solar metallicity and fixed microturbulence adequately models the stellar spectra
    Stellar parameters Teff, logg, vsini are derived by fitting to a TLUSTY grid with Z/Zsun=1, vmic=2 or 10 km/s, and no macroturbulence (Section 2.2.4). These assumptions affect HR positions and hence comparisons to instability regions.
  • domain assumption Frequencies below 0.5 d-1 are treated cautiously, not as coherent pulsations
    Section 2.4 notes that frequencies below 0.5 d-1 could be instrumental or rotational; classification prioritises consistent signals across sectors, which affects the SPB vs SLF split.
  • domain assumption Evolutionary tracks and GYRE instability regions from Burssens et al. (2020) are valid comparators
    Used in Figs. 2 and 5; the paper acknowledges the tracks are non-rotating and use a single convective boundary mixing prescription, making them representative but not perfect.
  • domain assumption The 4.0 sigma and 20 km/s thresholds separate binaries from pulsations
    Adopted from Sana et al.; the paper itself demonstrates these are ambiguous for galactic B-type pulsators (Section 5.3.2).
  • domain assumption Visual inspection correctly identifies all SB2 and emission-line stars
    Section 2.2.1 relies on visual inspection of H alpha and He I lines to remove SB2 and emission stars; missed systems would corrupt the clean-sample statistics.

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Cite this review

Pith. "Pith review of The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry." pith.science (2026). https://pith.science/paper/LTBQFB4M

@misc{pith2026260803383,
  author       = {Pith},
  title        = {Pith review of: The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/LTBQFB4M}},
  note         = {Machine review of arXiv:2608.03383}
}
abstract

A wide range of variability mechanisms exist among intermediate mass and massive stars, which are not yet fully understood. Using complementary data sources for a large population of B- and O-type stars, we aim to study the prevalence and interplay of different types of variability, including binarity, pulsation, and rotation, to prepare for future modelling. To this end, we analyse high-resolution HERMES spectra and 2-min cadence TESS photometry and characterise the diverse variability observed within a population of 873 O- and B-type stars. The spectroscopic data were normalised using machine-learning techniques, compared to a grid of synthetic TLUSTY spectra to determine stellar parameters, and used to identify radial velocity variability. Photometric time series were analysed using standard frequency analysis methods to detect pulsations and rotational modulation signatures. We find that more than 93 per cent of the sample exhibits photometric variability. Photometric variability caused by pulsations is identified in 82 per cent of the sample, with dominant contributions from $\beta$ Cep and slowly pulsating B-type stars, as well as stochastic low-frequency variability. Based on a limited number of spectroscopic epochs, at least 14 per cent of the stars show evidence of binarity, including both eclipsing and spectroscopic systems. This work represents one of the largest homogeneous surveys of variability for intermediate-mass and massive stars in the Northern hemisphere, and complementing similar efforts in the Southern hemisphere. It provides a statistical framework for future studies of stellar structure and evolution, particularly in the context of asteroseismology.

Figures

Figures reproduced from arXiv: 2608.03383 by the authors.

Figure 1
Figure 1. Distribution of spectral types from SIMBAD for the stars in our sample, classified by pulsator class from our analysis of TESS photometry, described in detail in Section 2.4. The spectroscopic data in this work were assembled with the High Efficiency and Resolution Mercator Echelle Spectrograph (HER￾MES; Raskin et al. 2011; Raskin & Van Winckel 2014). The HER￾MES instrument is a fibre-fed prism-cross-dispersed echel… view at source ↗
Figure 2
Figure 2. Spectroscopic HR diagrams for 322 stars in our sample with available stellar parameters from the Gaia ESP-HS database, which show our classifications based on HERMES spectroscopy (left) and TESS photometry (right). For both cases, we use the evolutionary tracks for a range of masses (solid grey lines) from Burssens et al. (2020). The zero-age main sequence (ZAMS) and terminal-age main sequence (TAMS) are denoted by … view at source ↗
Figure 3
Figure 3. Comparisons of stellar parameters from the Gaia ESP-HS database to those determined in this study using a grid-based fitting of TLUSTY atmospheric models. Targets have been labelled with respect to their photometric classification. Grey dashed lines corresponding to unity have been drawn for clarity, and an additional red-dashed line has been added for the Teff plot, representing a linear regression to the data poin… view at source ↗
Figures from the paper (6 more)
Figure 4
Figure 4. Figure 4: TESS light curves and Lomb-Scargle (LS) periodograms for four β Cep (blue; TIC 288489491, TIC 53968952, TIC 410521615 and TIC 304379819) and four SPB stars (red; TIC 236996722, TIC 213412439, TIC 198456386 and TIC 42062129). The LS periodograms show two different secto…
Figure 5
Figure 5. Figure 5: Spectroscopic HR diagram showing the distribution density of the three main pulsator types found in the sample (β Cep, SPB, and SLF). Contours are drawn at the 66th and 33rd percentiles in terms of population intervals for the hatched and filled regions, respectively. …
Figure 6
Figure 6. Figure 6: Distributions of v sin i values derived in this work from grid-based fitting of rotationally broadened TLUSTY atmospheric models for the three main pulsator types: 200 β Cep stars, 116 SPB stars, and 167 stars with SLF variability as their dominant type of photometric …
Figure 7
Figure 7. Figure 7: Top panel: Stacked distributions of the calculated ∆RV values for the three main types of pulsating star in the sample, in comparison to the EB population. Bottom panel: ∆RV value distribution for all targets in the sample that are not identified as a pulsator nor an E…
Figure 8
Figure 8. Figure 8: Comparison between calculated ∆RV values measured from multi￾epoch HERMES spectra versus the amplitude of the dominant pulsation frequency based on TESS data, which are divided into the three main pulsator types. The dashed grey line is simply a unity line (i.e. not a …
Figure 9
Figure 9. Figure 9: LS periodograms for four example stars showing rotational modu￾lation. In each case, the solid red line corresponds to the rotation frequency, and the dashed red line corresponds to its first harmonic (f = 2 × frot). The TIC ID of each star and its SIMBAD spectral type…

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Works this paper leans on

199 extracted references · 27 canonical work pages

  1. [1]

    , keywords =

    A gravitational-wave standard siren measurement of the Hubble constant. , keywords =. doi:10.1038/nature24471 , archivePrefix =. 1710.05835 , primaryClass =

    arXiv

  2. [2]

    , keywords =

    Multi-messenger Observations of a Binary Neutron Star Merger. , keywords =. doi:10.3847/2041-8213/aa91c9 , archivePrefix =. 1710.05833 , primaryClass =

    arXiv

  3. [3]

    , keywords =

    Collective pulsational velocity broadening due to gravity modes as a physical explanation for macroturbulence in hot massive stars. , keywords =. doi:10.1051/0004-6361/200810471 , archivePrefix =. 0909.3585 , primaryClass =

    arXiv

  4. [4]

    doi:10.1007/978-1-4020-5803-5 , adsurl =

    Asteroseismology. doi:10.1007/978-1-4020-5803-5 , adsurl =

    doi:10.1007/978-1-4020-5803-5

  5. [5]

    The young massive SMC cluster NGC 330 seen by MUSE. III. Stellar parameters and rotational velocities. , keywords =. doi:10.1051/0004-6361/202345950 , archivePrefix =. 2308.14799 , primaryClass =

    arXiv

  6. [6]

    , keywords =

    The Surface Nitrogen Abundance of a Massive Star in Relation to its Oscillations, Rotation, and Magnetic Field. , keywords =. doi:10.1088/0004-637X/781/2/88 , archivePrefix =. 1312.4144 , primaryClass =

    arXiv

  7. [7]

    , keywords =

    Observational Signatures of Convectively Driven Waves in Massive Stars. , keywords =. doi:10.1088/2041-8205/806/2/L33 , archivePrefix =. 1505.06648 , primaryClass =

    arXiv

  8. [8]

    Reviews of Modern Physics , keywords =

    Probing the interior physics of stars through asteroseismology. Reviews of Modern Physics , keywords =. doi:10.1103/RevModPhys.93.015001 , archivePrefix =. 1912.12300 , primaryClass =

    arXiv 1912

Show all 199 references
  1. [9]

    A big step forward: introducing numerical models including a stellar mass-loss

    Time-dependent atomic diffusion in the atmospheres of CP stars. A big step forward: introducing numerical models including a stellar mass-loss. , keywords =. doi:10.1093/mnras/sty3003 , archivePrefix =. 1811.02267 , primaryClass =

    arXiv

  2. [10]

    Nature Astronomy , keywords =

    The photometric variability of massive stars due to gravity waves excited by core convection. Nature Astronomy , keywords =. doi:10.1038/s41550-023-02040-7 , archivePrefix =. 2306.08023 , primaryClass =

    arXiv

  3. [12]

    , keywords =

    The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package. , keywords =. doi:10.3847/1538-3881/aabc4f , archivePrefix =. 1801.02634 , primaryClass =

    arXiv

  4. [13]

    Evidence for a dipole field lower limit and a tentative interpretation of the magnetic dichotomy

    Weak magnetic fields in Ap/Bp stars. Evidence for a dipole field lower limit and a tentative interpretation of the magnetic dichotomy. , keywords =. doi:10.1051/0004-6361:20078189 , archivePrefix =. 0710.1554 , primaryClass =

    arXiv

  5. [14]

    10.1051/0004-6361/200810860

    The CoRoT satellite in flight: description and performance* , DOI= "10.1051/0004-6361/200810860", url= "https://doi.org/10.1051/0004-6361/200810860", journal =

    doi

  6. [15]

    Astronomische Nachrichten , keywords =

    Eclipsing variables: Catalogue and classification. Astronomische Nachrichten , keywords =. doi:10.1002/asna.201311942 , adsurl =

    doi

  7. [16]

    Short-term variability and mass loss in Be stars. I. BRITE satellite photometry of and Centauri. , keywords =. doi:10.1051/0004-6361/201528026 , archivePrefix =. 1602.01744 , primaryClass =

    arXiv

  8. [17]

    Pre-launch description

    The Gaia astrophysical parameters inference system (Apsis). Pre-launch description. , keywords =. doi:10.1051/0004-6361/201322344 , archivePrefix =. 1309.2157 , primaryClass =

    arXiv

  9. [18]

    , keywords =

    The observed multiplicity properties of B-type stars in the Galactic young open cluster NGC 6231. , keywords =. doi:10.1051/0004-6361/202141037 , archivePrefix =. 2108.07814 , primaryClass =

    arXiv

  10. [19]

    HD 46223, HD 46150, and HD 46966

    Variability in the CoRoT photometry of three hot O-type stars. HD 46223, HD 46150, and HD 46966. , keywords =. doi:10.1051/0004-6361/201116949 , archivePrefix =. 1107.0267 , primaryClass =

    arXiv

  11. [20]

    Science , keywords =

    Kepler Planet-Detection Mission: Introduction and First Results. Science , keywords =. doi:10.1126/science.1185402 , adsurl =

    doi

  12. [21]

    arXiv , author =:2006.13229 , journal =

    doi:10.1051/0004-6361/202037640 , eid =. arXiv , author =:2006.13229 , journal =

    2006 arXiv

  13. [22]

    The young massive SMC cluster NGC 330 seen by MUSE. II. Multiplicity properties of the massive-star population. , keywords =. doi:10.1051/0004-6361/202140507 , archivePrefix =. 2104.13409 , primaryClass =

    arXiv

  14. [23]

    , keywords =

    Binarity at LOw Metallicity (BLOeM): Multiplicity properties of Oe and Be stars. , keywords =. doi:10.1051/0004-6361/202452623 , archivePrefix =. 2502.02641 , primaryClass =

    arXiv

  15. [24]

    , keywords =

    K2 space photometry reveals rotational modulation and stellar pulsations in chemically peculiar A and B stars. , keywords =. doi:10.1051/0004-6361/201833037 , archivePrefix =. 1805.01799 , primaryClass =

    arXiv

  16. [25]

    Nature Astronomy , keywords =

    Low-frequency gravity waves in blue supergiants revealed by high-precision space photometry. Nature Astronomy , keywords =. doi:10.1038/s41550-019-0768-1 , archivePrefix =. 1905.02120 , primaryClass =

    1905 arXiv

  17. [26]

    , keywords =

    Discovery of Tidally Perturbed Pulsations in the Eclipsing Binary U Gru: A Crucial System for Tidal Asteroseismology. , keywords =. doi:10.3847/2041-8213/ab3fb2 , archivePrefix =. 1908.08468 , primaryClass =

    arXiv

  18. [27]

    Frontiers in Astronomy and Space Sciences , keywords =

    Asteroseismology of high-mass stars: new insights of stellar interiors with space telescopes. Frontiers in Astronomy and Space Sciences , keywords =. doi:10.3389/fspas.2020.578584 , archivePrefix =. 2008.11162 , primaryClass =

    2020

  19. [28]

    Photometric detection of internal gravity waves in upper main-sequence stars. II. Combined TESS photometry and high-resolution spectroscopy. , keywords =. doi:10.1051/0004-6361/202038224 , archivePrefix =. 2006.03012 , primaryClass =

    2006 arXiv

  20. [29]

    The CubeSpec space mission. I. Asteroseismology of massive stars from time-series optical spectroscopy: Science requirements and target list prioritisation. , keywords =. doi:10.1051/0004-6361/202142375 , archivePrefix =. 2111.09814 , primaryClass =

    arXiv

  21. [30]

    Science , keywords =

    A magnetic massive star has experienced a stellar merger. Science , keywords =. doi:10.1126/science.adg7700 , archivePrefix =. 2404.10167 , primaryClass =

    arXiv

  22. [31]

    , keywords =

    Stellar mergers as the origin of magnetic massive stars. , keywords =. doi:10.1038/s41586-019-1621-5 , archivePrefix =. 1910.14058 , primaryClass =

    1910 arXiv

  23. [32]

    Encyclopedia of Astrophysics, Volume 2 , year = 2026, volume =

    Stellar magnetism. Encyclopedia of Astrophysics, Volume 2 , year = 2026, volume =. doi:10.1016/B978-0-443-21439-4.00074-2 , adsurl =

    2026 doi

  24. [33]

    , keywords =

    Angular Momentum Transport in Stellar Interiors. , keywords =. doi:10.1146/annurev-astro-091918-104359 , archivePrefix =. 1809.07779 , primaryClass =

    arXiv

  25. [34]

    doi:10.1007/978-3-319-66649-5 , adsurl =

    Amplitude Modulation of Pulsation Modes in Delta Scuti Stars. doi:10.1007/978-3-319-66649-5 , adsurl =

    doi

  26. [35]

    doi:10.1093/mnrasl/slv142 , eprint =

    , keywords =. doi:10.1093/mnrasl/slv142 , eprint =

    doi

  27. [36]

    doi:10.1093/mnras/staa1292 , eprint =

    , keywords =. doi:10.1093/mnras/staa1292 , eprint =

    doi

  28. [37]

    doi:10.1553/cia159s42 , journal =

    doi

  29. [38]

    , keywords =

    MOST Detects g- and p-Modes in the B Supergiant HD 163899 (B2 Ib/II). , keywords =. doi:10.1086/507409 , archivePrefix =. astro-ph/0606712 , primaryClass =

    arXiv

  30. [39]

    arXiv , author =:2104.06278 , journal =

    doi:10.1051/0004-6361/202040105 , eid =. arXiv , author =:2104.06278 , journal =

    arXiv

  31. [40]

    , keywords =

    The Potential of Asteroseismology to Resolve the Blue Supergiant Problem. , keywords =. doi:10.3847/2041-8213/ad4990 , archivePrefix =. 2311.00038 , primaryClass =

    arXiv

  32. [41]

    ''The Observation and Analysis of Stellar Photospheres, 3rd Edition, by D.F. Gray. ISBN 0521851866. <A href=''http://www.cambridge.org/us/catalogue/catalogue.asp?isbn=0521851866. Cambridge''>http://www.cambridge.org/us/catalogue/catalogue.asp?isbn=0521851866. Cambridge</A>, UK...

    2005

  33. [42]

    Photometric detection of internal gravity waves in upper main-sequence stars. III. Comparison of amplitude spectrum fitting and Gaussian process regression using CELERITE2. , keywords =. doi:10.1051/0004-6361/202243545 , archivePrefix =. 2211.08347 , primaryClass =

    arXiv

  34. [43]

    , keywords =

    Making waves in massive star asteroseismology. , keywords =. doi:10.1007/s10509-023-04262-7 , archivePrefix =. 2312.08319 , primaryClass =

    arXiv

  35. [44]

    Comparable stochastic low-frequency variability in SMC, LMC, and Galactic massive stars

    Photometric detection of internal gravity waves in upper main-sequence stars: IV. Comparable stochastic low-frequency variability in SMC, LMC, and Galactic massive stars. , keywords =. doi:10.1051/0004-6361/202451419 , archivePrefix =. 2410.12726 , primaryClass =

    arXiv

  36. [45]

    , keywords =

    A fossil origin for the magnetic field in A stars and white dwarfs. , keywords =. doi:10.1038/nature02934 , archivePrefix =. astro-ph/0502043 , primaryClass =

    arXiv

  37. [46]

    , keywords =

    Stable magnetic fields in stellar interiors. , keywords =. doi:10.1051/0004-6361:20041980 , archivePrefix =. astro-ph/0510316 , primaryClass =

    arXiv

  38. [47]

    Astrocut: Tools for creating cutouts of TESS images

  39. [48]

    , keywords =

    The First Stars. , keywords =. doi:10.1146/annurev.astro.42.053102.134034 , archivePrefix =. astro-ph/0311019 , primaryClass =

  40. [49]

    , keywords =

    Binarity at LOw Metallicity (BLOeM): Multiplicity of early B-type supergiants in the Small Magellanic Cloud. , keywords =. doi:10.1051/0004-6361/202452963 , archivePrefix =. 2502.12239 , primaryClass =

    arXiv

  41. [50]

    , keywords =

    Variability of OB stars from TESS southern Sectors 1-13 and high-resolution IACOB and OWN spectroscopy. , keywords =. doi:10.1051/0004-6361/202037700 , archivePrefix =. 2005.09658 , primaryClass =

    2005 arXiv

  42. [51]

    Nature Astronomy , keywords =

    A calibration point for stellar evolution from massive star asteroseismology. Nature Astronomy , keywords =. doi:10.1038/s41550-023-01978-y , archivePrefix =. 2306.11798 , primaryClass =

    arXiv

  43. [52]

    , keywords =

    Detection of magnetic fields in chemically peculiar stars observed with the K2 space mission. , keywords =. doi:10.1093/mnras/sty1190 , archivePrefix =. 1805.00781 , primaryClass =

    arXiv

  44. [53]

    , keywords =

    Forward seismic modeling of the pulsating magnetic B-type star HD 43317. , keywords =. doi:10.1051/0004-6361/201832642 , archivePrefix =. 1805.00802 , primaryClass =

    arXiv

  45. [54]

    , keywords =

    On the Origin of Stochastic, Low-Frequency Photometric Variability in Massive Stars. , keywords =. doi:10.3847/1538-4357/ac03b0 , archivePrefix =. 2102.05670 , primaryClass =

    arXiv

  46. [55]

    , keywords =

    The spectroscopic Hertzsprung-Russell diagram of Galactic massive stars. , keywords =. doi:10.1051/0004-6361/201425028 , archivePrefix =. 1410.3499 , primaryClass =

    arXiv

  47. [56]

    , keywords =

    Asteroseismology of Solar-Type and Red-Giant Stars. , keywords =. doi:10.1146/annurev-astro-082812-140938 , archivePrefix =. 1303.1957 , primaryClass =

    1957 arXiv

  48. [57]

    , keywords =

    Detection of Scuti Pulsators in the Eclipsing Binaries Observed by TESS. , keywords =. doi:10.3847/1538-4365/aca284 , archivePrefix =. 2211.05283 , primaryClass =

    arXiv

  49. [58]

    RAA , year = 2012, month = sep, volume =

    The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST). RAA , year = 2012, month = sep, volume =. doi:10.1088/1674-4527/12/9/003 , adsurl =

    2012 doi

  50. [59]

    New clues on the location of the TAMS in the massive star domain

    The IACOB project: XIV. New clues on the location of the TAMS in the massive star domain. , keywords =. doi:10.1051/0004-6361/202453242 , archivePrefix =. 2501.17984 , primaryClass =

    arXiv

  51. [60]

    A study of bright southern slowly pulsating B stars. III. Mode identification for singly-periodic targets in spectroscopy. , keywords =. doi:10.1051/0004-6361:20042103 , adsurl =

    doi

  52. [61]

    Frequencies and mode identification of variable O-B stars

    Long term photometric monitoring with the Mercator telescope. Frequencies and mode identification of variable O-B stars. , keywords =. doi:10.1051/0004-6361:20066202 , adsurl =

    doi

  53. [62]

    , keywords =

    The Rotation Rates of Massive Stars: The Role of Binary Interaction through Tides, Mass Transfer, and Mergers. , keywords =. doi:10.1088/0004-637X/764/2/166 , archivePrefix =. 1211.3742 , primaryClass =

    arXiv

  54. [63]

    , keywords =

    Magnetic Fields of Nondegenerate Stars. , keywords =. doi:10.1146/annurev-astro-082708-101833 , archivePrefix =. 0904.1938 , primaryClass =

    1938 arXiv

  55. [64]

    A spectroscopic multiplicity survey of Galactic Wolf-Rayet stars. I. The northern WC sequence. , keywords =. doi:10.1051/0004-6361/202038446 , archivePrefix =. 2006.13957 , primaryClass =

    2006 arXiv

  56. [65]

    The VLT-FLAMES Tarantula Survey. XXII. Multiplicity properties of the B-type stars. , keywords =. doi:10.1051/0004-6361/201526192 , archivePrefix =. 1505.07121 , primaryClass =

    arXiv

  57. [66]

    Three-dimensional Simulations of Massive Stars. I. Wave Generation and Propagation. , keywords =. doi:10.3847/1538-4357/ab12df , archivePrefix =. 1903.09392 , primaryClass =

    1903 arXiv

  58. [67]

    Grids of stellar models with rotation. I. Models from 0.8 to 120 M _ at solar metallicity (Z = 0.014). , keywords =. doi:10.1051/0004-6361/201117751 , archivePrefix =. 1110.5049 , primaryClass =

    arXiv

  59. [68]

    , keywords =

    Binary Population and Spectral Synthesis Version 2.1: Construction, Observational Verification, and New Results. , keywords =. doi:10.1017/pasa.2017.51 , archivePrefix =. 1710.02154 , primaryClass =

    2017 arXiv

  60. [69]

    , keywords =

    First Observation of the Complete Rotation Period of the Ultraslowly Rotating Magnetic O Star HD 54879. , keywords =. doi:10.3847/1538-4357/ad865a , archivePrefix =. 2401.09722 , primaryClass =

    arXiv

  61. [70]

    , keywords =

    Cephei Pulsators in Eclipsing Binaries Observed with TESS. , keywords =. doi:10.3847/1538-4365/ad39c5 , archivePrefix =. 2403.12281 , primaryClass =

    arXiv

  62. [71]

    Gaia Data Release 3. Apsis. II. Stellar parameters. , keywords =. doi:10.1051/0004-6361/202243919 , archivePrefix =. 2206.05992 , primaryClass =

    arXiv

  63. [72]

    EES2023: Proceedings of the Evry Schatzman School , year = 2024, editor =

    Astrophysical Parameters associated to 'Hot' stars in Gaia DR3. EES2023: Proceedings of the Evry Schatzman School , year = 2024, editor =. doi:10.48550/arXiv.2411.04887 , archivePrefix =. 2411.04887 , primaryClass =

    2024 doi arXiv

  64. [73]

    , keywords =

    Mode identification and ensemble asteroseismology of 119 Cep stars detected by Gaia light curves and monitored by TESS. , keywords =. doi:10.1051/0004-6361/202451721 , archivePrefix =. 2408.06097 , primaryClass =

    arXiv

  65. [74]

    , keywords =

    An interferometric study of B star multiplicity. , keywords =. doi:10.1051/0004-6361/202554344 , archivePrefix =. 2505.02300 , primaryClass =

    arXiv

  66. [75]

    Summary of the content and survey properties

    Gaia Data Release 3. Summary of the content and survey properties. , keywords =. doi:10.1051/0004-6361/202243940 , archivePrefix =. 2208.00211 , primaryClass =

    arXiv

  67. [76]

    A golden sample of astrophysical parameters

    Gaia Data Release 3. A golden sample of astrophysical parameters. , keywords =. doi:10.1051/0004-6361/202243800 , archivePrefix =. 2206.05870 , primaryClass =

    arXiv

  68. [77]

    , keywords =

    The excess of cool supergiants from contemporary stellar evolution models defies the metallicity-independent Humphreys-Davidson limit. , keywords =. doi:10.1093/mnras/stab383 , archivePrefix =. 2102.03102 , primaryClass =

    arXiv

  69. [78]

    , keywords =

    The MiMeS survey of Magnetism in Massive Stars: magnetic analysis of the O-type stars. , keywords =. doi:10.1093/mnras/stw2743 , archivePrefix =. 1610.07895 , primaryClass =

    arXiv

  70. [79]

    , keywords =

    Giant star seismology. , keywords =. doi:10.1007/s00159-017-0101-x , archivePrefix =. 1609.07487 , primaryClass =

    arXiv

  71. [80]

    , keywords =

    Confronting sparse Gaia DR3 photometry with TESS for a sample of around 60 000 OBAF-type pulsators. , keywords =. doi:10.1051/0004-6361/202450489 , archivePrefix =. 2405.01539 , primaryClass =

    arXiv

  72. [81]

    The B0.5IVe CoRoT target HD 49330. I. Photometric analysis from CoRoT data. , keywords =. doi:10.1051/0004-6361/200911928 , adsurl =

    doi

  73. [82]

    Non-LTE Line-blanketed Model Atmospheres of Hot Stars. I. Hybrid Complete Linearization/Accelerated Lambda Iteration Method. , keywords =. doi:10.1086/175226 , adsurl =

    doi

  74. [83]

    10.1051/0004-6361/202037750

    A plethora of new, magnetic chemically peculiar stars from LAMOST DR4 , DOI= "10.1051/0004-6361/202037750", url= "https://doi.org/10.1051/0004-6361/202037750", journal =

    doi

  75. [84]

    , keywords =

    An all-sky sample of intermediate- to high-mass OBA-type eclipsing binaries observed by TESS. , keywords =. doi:10.1051/0004-6361/202141489 , archivePrefix =. 2107.10005 , primaryClass =

    arXiv

  76. [85]

    Software and Cyberinfrastructure for Astronomy IV , year = 2016, editor =

    The TESS science processing operations center. Software and Cyberinfrastructure for Astronomy IV , year = 2016, editor =. doi:10.1117/12.2233418 , adsurl =

    2016 doi

  77. [86]

    , keywords =

    Large-scale variability in macroturbulence driven by pulsations in the rapidly rotating massive star Oph from high-cadence ESPRESSO spectroscopy and TESS photometry. , keywords =. doi:10.1051/0004-6361/202555936 , archivePrefix =. 2509.09635 , primaryClass =

  78. [87]

    Implementation of magnetic braking in MESA and implications for the evolution of surface rotation in OB stars

    The effects of surface fossil magnetic fields on massive star evolution - II. Implementation of magnetic braking in MESA and implications for the evolution of surface rotation in OB stars. , keywords =. doi:10.1093/mnras/staa237 , archivePrefix =. 2001.06239 , primaryClass =

    2001 arXiv

  79. [88]

    Effects of the individual abundance patterns

    Theoretical analysis of the atmospheres of CP stars. Effects of the individual abundance patterns. , keywords =. doi:10.1051/0004-6361:20077192 , archivePrefix =. 0706.4028 , primaryClass =

    arXiv

  80. [89]

    , keywords =

    Multi-element abundance Doppler imaging of the rapidly oscillating Ap star HR 3831. , keywords =. doi:10.1051/0004-6361:20040517 , adsurl =

    doi

  81. [90]

    Numerical tests and assessment of systematic errors

    Doppler imaging of chemical spots on magnetic Ap/Bp stars. Numerical tests and assessment of systematic errors. , keywords =. doi:10.1051/0004-6361/201629768 , archivePrefix =. 1611.05473 , primaryClass =

    arXiv

  82. [91]

    , keywords =

    Light variations due to the line-driven wind instability and wind blanketing in O stars. , keywords =. doi:10.1051/0004-6361/201731614 , archivePrefix =. 1807.09407 , primaryClass =

    arXiv

  83. [92]

    , keywords =

    Stochastic light variations in hot stars from wind instability: finding photometric signatures and testing against the TESS data. , keywords =. doi:10.1051/0004-6361/202040148 , archivePrefix =. 2103.08755 , primaryClass =

    arXiv

  84. [93]

    Synthetic a photometry: the normality line

    The 5200- A flux depression of chemically peculiar stars - I. Synthetic a photometry: the normality line. , keywords =. doi:10.1046/j.1365-8711.2003.06452.x , archivePrefix =. astro-ph/0303225 , primaryClass =

    2003

  85. [94]

    The cool chemically peculiar and Bootis stars

    The 5200- A flux depression of chemically peculiar stars - II. The cool chemically peculiar and Bootis stars. , keywords =. doi:10.1111/j.1365-2966.2004.07977.x , adsurl =

    2004

  86. [95]

    , keywords =

    A unifying explanation of complex frequency spectra of Dor, SPB and Be stars: combination frequencies and highly non-sinusoidal light curves. , keywords =. doi:10.1093/mnras/stv868 , archivePrefix =. 1504.04245 , primaryClass =

    arXiv

  87. [96]

    , year = 2022, month = aug, volume =

    Asteroseismology Across the Hertzsprung-Russell Diagram. , year = 2022, month = aug, volume =. doi:10.1146/annurev-astro-052920-094232 , adsurl =

    2022 doi

  88. [97]

    , keywords =

    Outbursts and Disk Variability in Be Stars. , keywords =. doi:10.3847/1538-3881/aa9c7e , archivePrefix =. 1708.02594 , primaryClass =

    arXiv

  89. [98]

    Classifying Be Star Variability With TESS. I. The Southern Ecliptic. , keywords =. doi:10.3847/1538-3881/ac5abd , archivePrefix =. 2010.13905 , primaryClass =

    2010 arXiv

  90. [99]

    From localized ejection to circularization

    The birth of Be star disks: I. From localized ejection to circularization. , keywords =. doi:10.1051/0004-6361/202453321 , archivePrefix =. 2504.07571 , primaryClass =

    arXiv

  91. [100]

    , keywords =

    Presupernova Evolution of Massive Single and Binary Stars. , keywords =. doi:10.1146/annurev-astro-081811-125534 , archivePrefix =. 1206.5443 , primaryClass =

    arXiv

  92. [101]

    , keywords =

    The spectroscopic Hertzsprung-Russell diagram. , keywords =. doi:10.1051/0004-6361/201423374 , archivePrefix =. 1403.2212 , primaryClass =

    arXiv

  93. [102]

    , keywords =

    A Grid of Non-LTE Line-blanketed Model Atmospheres of O-Type Stars. , keywords =. doi:10.1086/374373 , archivePrefix =. astro-ph/0210157 , primaryClass =

    arXiv

  94. [103]

    , keywords =

    A Grid of NLTE Line-blanketed Model Atmospheres of Early B-Type Stars. , keywords =. doi:10.1086/511270 , archivePrefix =. astro-ph/0611891 , primaryClass =

    arXiv

  95. [104]

    , keywords =

    The expansion of stripped-envelope stars: Consequences for supernovae and gravitational-wave progenitors. , keywords =. doi:10.1051/0004-6361/201937300 , archivePrefix =. 2003.01120 , primaryClass =

    2003 arXiv

  96. [105]

    , keywords =

    Asteroseismic inference of the near-core magnetic field strength in the main-sequence B star HD 43317. , keywords =. doi:10.1093/mnrasl/slac013 , archivePrefix =. 2202.03440 , primaryClass =

    arXiv

  97. [106]

    , keywords =

    New Oe Stars in LAMOST DR5. , keywords =. doi:10.3847/1538-4357/aad04f , archivePrefix =. 1807.00574 , primaryClass =

    arXiv

  98. [107]

    , keywords =

    Galactic O-type Stars in LAMOST Data. , keywords =. doi:10.3847/1538-4365/abe716 , archivePrefix =. 2103.13874 , primaryClass =

    arXiv

  99. [108]

    Lightkurve: Kepler and TESS time series analysis in Python

  100. [109]

    , keywords =

    Least-Squares Frequency Analysis of Unequally Spaced Data. , keywords =. doi:10.1007/BF00648343 , adsurl =

    doi

  101. [110]

    , keywords =

    A catalogue of eclipsing variables. , keywords =. doi:10.1051/0004-6361:20053137 , adsurl =

    doi

  102. [111]

    , keywords =

    Properties of six short-period massive binaries: A study of the effects of binarity on surface chemical abundances. , keywords =. doi:10.1051/0004-6361/201731593 , archivePrefix =. 1709.00937 , primaryClass =

    arXiv

  103. [112]

    The Tarantula Massive Binary Monitoring. III. Atmosphere analysis of double-lined spectroscopic systems. , keywords =. doi:10.1051/0004-6361/201936151 , archivePrefix =. 1912.08107 , primaryClass =

    1912 arXiv

  104. [113]

    , keywords =

    Multiplicity of Galactic luminous blue variable stars. , keywords =. doi:10.1051/0004-6361/202040062 , archivePrefix =. 2105.12380 , primaryClass =

    arXiv

  105. [114]

    , keywords =

    A comparison of evolutionary tracks for single Galactic massive stars. , keywords =. doi:10.1051/0004-6361/201322480 , archivePrefix =. 1310.7218 , primaryClass =

    arXiv

  106. [115]

    Stellar evolution with rotation. V. Changes in all the outputs of massive star models. , keywords =. doi:10.48550/arXiv.astro-ph/0006404 , archivePrefix =. astro-ph/0006404 , primaryClass =

    doi arXiv

  107. [116]

    , keywords =

    Photoelectric filter photometry of the lambda 5200 flux depression in Ap-stars. , keywords =

  108. [117]

    , keywords =

    The Evolution of Massive Binary Stars. , keywords =. doi:10.1146/annurev-astro-052722-105936 , archivePrefix =. 2311.01865 , primaryClass =

    arXiv

  109. [118]

    , year = 2003, month = jan, volume =

    MASSIVE STARS IN THE LOCAL GROUP: Implications for Stellar Evolution and Star Formation. , year = 2003, month = jan, volume =. doi:10.1146/annurev.astro.41.071601.170033 , adsurl =

    2003

  110. [119]

    , keywords =

    Long-period Ap stars discovered with TESS data. , keywords =. doi:10.1051/0004-6361/202038007 , archivePrefix =. 2003.14144 , primaryClass =

    2003 arXiv

  111. [120]

    , keywords =

    The S _ B ^ 9 catalogue: status, comparison with non-single stars from Gaia DR3, and evolution to S _ B ^ X. , keywords =. doi:10.1093/mnras/stag351 , archivePrefix =. 2602.17870 , primaryClass =

  112. [121]

    , year = 1970, month = may, volume =

    Diffusion Processes in Peculiar a Stars. , year = 1970, month = may, volume =. doi:10.1086/150459 , adsurl =

    1970 doi

  113. [122]

    , keywords =

    Diffusion models for magnetic Ap-Bp stars. , keywords =

  114. [123]

    , keywords =

    Mind Your Ps and Qs: The Interrelation between Period (P) and Mass-ratio (Q) Distributions of Binary Stars. , keywords =. doi:10.3847/1538-4365/aa6fb6 , archivePrefix =. 1606.05347 , primaryClass =

    arXiv

  115. [124]

    The first Gaia catalogue of eclipsing-binary candidates

    Gaia Data Release 3. The first Gaia catalogue of eclipsing-binary candidates. , keywords =. doi:10.1051/0004-6361/202245330 , archivePrefix =. 2211.00929 , primaryClass =

    arXiv

  116. [125]

    Stellar content and binary properties

    Characterization of B-type stars in four young Galactic open clusters I. Stellar content and binary properties. , keywords =. doi:10.1093/mnras/staf809 , archivePrefix =. 2505.08955 , primaryClass =

    arXiv

  117. [126]

    A comprehensive study of nearby early B-type stars and implications for stellar and Galactic evolution and interstellar dust models

    Present-day cosmic abundances. A comprehensive study of nearby early B-type stars and implications for stellar and Galactic evolution and interstellar dust models. , keywords =. doi:10.1051/0004-6361/201118158 , archivePrefix =. 1203.5787 , primaryClass =

    arXiv

  118. [127]

    Protostars and Planets VII , year = 2023, editor =

    The Origin and Evolution of Multiple Star Systems. Protostars and Planets VII , year = 2023, editor =. doi:10.48550/arXiv.2203.10066 , archivePrefix =. 2203.10066 , primaryClass =

    2023 doi arXiv

  119. [128]

    Internal gravity waves matter for SLF variability

    3D hydrodynamic simulations of massive main-sequence stars -- IV. Internal gravity waves matter for SLF variability. arXiv e-prints , keywords =. doi:10.48550/arXiv.2508.03893 , archivePrefix =. 2508.03893 , primaryClass =

    doi

  120. [129]

    , keywords =

    Binarity at LOw Metallicity (BLOeM): The multiplicity properties and evolution of BAF-type supergiants. , keywords =. doi:10.1051/0004-6361/202452949 , archivePrefix =. 2502.02644 , primaryClass =

    arXiv

  121. [130]

    , keywords =

    On the detection of chemically peculiar stars using a photometry. , keywords =. doi:10.1051/0004-6361:20053001 , archivePrefix =. astro-ph/0507124 , primaryClass =

    arXiv

  122. [131]

    The eclipsing binary V453Cygni

    Chemical evolution of high-mass stars in close binaries - I. The eclipsing binary V453Cygni. , keywords =. doi:10.1111/j.1365-2966.2009.14418.x , archivePrefix =. 0812.3769 , primaryClass =

    2009

  123. [132]

    , keywords =

    Modules for Experiments in Stellar Astrophysics (MESA). , keywords =. doi:10.1088/0067-0049/192/1/3 , archivePrefix =. 1009.1622 , primaryClass =

    arXiv

  124. [133]

    , keywords =

    Modules for Experiments in Stellar Astrophysics (MESA): Planets, Oscillations, Rotation, and Massive Stars. , keywords =. doi:10.1088/0067-0049/208/1/4 , archivePrefix =. 1301.0319 , primaryClass =

    arXiv

  125. [134]

    , keywords =

    Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions. , keywords =. doi:10.1088/0067-0049/220/1/15 , archivePrefix =. 1506.03146 , primaryClass =

    arXiv

  126. [135]

    , keywords =

    Modules for Experiments in Stellar Astrophysics (MESA): Convective Boundaries, Element Diffusion, and Massive Star Explosions. , keywords =. doi:10.3847/1538-4365/aaa5a8 , archivePrefix =. 1710.08424 , primaryClass =

    arXiv

  127. [136]

    , keywords =

    Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation. , keywords =. doi:10.3847/1538-4365/ab2241 , archivePrefix =. 1903.01426 , primaryClass =

    1903 arXiv

  128. [137]

    Nature Astronomy , keywords =

    Internal mixing of rotating stars inferred from dipole gravity modes. Nature Astronomy , keywords =. doi:10.1038/s41550-021-01351-x , archivePrefix =. 2105.04533 , primaryClass =

    arXiv

  129. [138]

    , keywords =

    Internal Rotation and Inclinations of Slowly Pulsating B Stars: Evidence of Interior Angular Momentum Transport. , keywords =. doi:10.3847/1538-4357/ac947f , archivePrefix =. 2208.14497 , primaryClass =

    arXiv

  130. [139]

    , keywords =

    Stochastic low-frequency variability of 50 massive stars in the Cygnus OB associations and the Small Magellanic Cloud. , keywords =. doi:10.1093/mnras/staf661 , archivePrefix =. 2504.15861 , primaryClass =

    arXiv

  131. [140]

    , keywords =

    S _ B ^ 9 : The ninth catalogue of spectroscopic binary orbits. , keywords =. doi:10.1051/0004-6361:20041213 , archivePrefix =. astro-ph/0406573 , primaryClass =

    arXiv

  132. [141]

    , keywords =

    The chemically peculiar stars of the upper main sequence. , keywords =. doi:10.1146/annurev.aa.12.090174.001353 , adsurl =

  133. [142]

    TESS Eclipsing Binary Stars. I. Short-cadence Observations of 4584 Eclipsing Binaries in Sectors 1-26. , keywords =. doi:10.3847/1538-4365/ac324a , archivePrefix =. 2110.13382 , primaryClass =

    arXiv

  134. [143]

    , keywords =

    HERMES: a high-resolution fibre-fed spectrograph for the Mercator telescope. , keywords =. doi:10.1051/0004-6361/201015435 , archivePrefix =. 1011.0258 , primaryClass =

    arXiv

  135. [144]

    Astronomische Nachrichten , keywords =

    HERMES at Mercator, competitive high-resolution spectroscopy with a small telescope. Astronomische Nachrichten , keywords =. doi:10.1002/asna.201312009 , archivePrefix =. 1310.5235 , primaryClass =

    arXiv

  136. [145]

    Experimental Astronomy , keywords =

    The PLATO mission. Experimental Astronomy , keywords =. doi:10.1007/s10686-025-09985-9 , archivePrefix =. 2406.05447 , primaryClass =

    arXiv

  137. [146]

    Transiting Exoplanet Survey Satellite (TESS). J. Astron. Telesc. Instrum. Syst. , year = 2015, month = jan, volume =. doi:10.1117/1.JATIS.1.1.014003 , adsurl =

    2015 doi

  138. [147]

    Rapidly rotating B stars with viscous Keplerian decretion disks

    Classical Be stars. Rapidly rotating B stars with viscous Keplerian decretion disks. , keywords =. doi:10.1007/s00159-013-0069-0 , archivePrefix =. 1310.3962 , primaryClass =

    arXiv

  139. [148]

    Short-term variability and mass loss in Be stars. II. Physical taxonomy of photometric variability observed by the Kepler spacecraft. , keywords =. doi:10.1051/0004-6361/201628411 , archivePrefix =. 1608.02872 , primaryClass =

    arXiv

  140. [149]

    Encyclopedia of Astrophysics , year = 2026, volume =

    Classical Be stars. Encyclopedia of Astrophysics , year = 2026, volume =. doi:10.1016/B978-0-443-21439-4.00042-0 , archivePrefix =. 2411.06882 , primaryClass =

    2026

  141. [150]

    , keywords =

    Internal Gravity Waves in Massive Stars: Angular Momentum Transport. , keywords =. doi:10.1088/0004-637X/772/1/21 , archivePrefix =. 1306.3262 , primaryClass =

    arXiv

  142. [151]

    , keywords =

    On the Chemical Mixing Induced by Internal Gravity Waves. , keywords =. doi:10.3847/2041-8213/aa8d13 , archivePrefix =. 1709.04920 , primaryClass =

    arXiv

  143. [152]

    Results of Magnetic-Field Measurements with the 6-m Telescope. VI. Observations in 2012. Astrophysical Bulletin , keywords =. doi:10.1134/S1990341320030104 , adsurl =

    2012 doi

  144. [153]

    Research in Astronomy and Astrophysics , keywords =

    A Catalog and Statistical Analysis for Magnetic Stars. Research in Astronomy and Astrophysics , keywords =. doi:10.1088/1674-4527/ace9b0 , archivePrefix =. 2307.12315 , primaryClass =

    arXiv

  145. [154]

    Modelling of Stellar Atmospheres , year = 2003, editor =

    Observational Evidence for the Stratification of Chemical Abundances in Stellar Atmospheres. Modelling of Stellar Atmospheres , year = 2003, editor =

    2003

  146. [155]

    , keywords =

    Convective core entrainment in 1D main-sequence stellar models. , keywords =. doi:10.1093/mnras/stab752 , archivePrefix =. 2103.06196 , primaryClass =

    arXiv

  147. [156]

    Science , keywords =

    Binary Interaction Dominates the Evolution of Massive Stars. Science , keywords =. doi:10.1126/science.1223344 , archivePrefix =. 1207.6397 , primaryClass =

    arXiv

  148. [157]

    The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population. , keywords =. doi:10.1051/0004-6361/201219621 , archivePrefix =. 1209.4638 , primaryClass =

    arXiv

  149. [158]

    Nature Astronomy , keywords =

    A high fraction of close massive binary stars at low metallicity. Nature Astronomy , keywords =. doi:10.1038/s41550-025-02610-x , archivePrefix =. 2509.12488 , primaryClass =

  150. [159]

    Studies in astronomical time series analysis. II. Statistical aspects of spectral analysis of unevenly spaced data. , keywords =. doi:10.1086/160554 , adsurl =

    doi

  151. [160]

    , keywords =

    Asteroseismology of SPB stars: a comparison of forward asteroseismic modelling results from Kepler and TESS. , keywords =. doi:10.1093/mnras/staf2174 , archivePrefix =. 2512.05864 , primaryClass =

  152. [161]

    Spectroscopy, orbital analysis, formation, and evolution

    The Wolf-Rayet binaries of the nitrogen sequence in the Large Magellanic Cloud. Spectroscopy, orbital analysis, formation, and evolution. , keywords =. doi:10.1051/0004-6361/201935684 , archivePrefix =. 1905.09296 , primaryClass =

    1905 arXiv

  153. [162]

    , keywords =

    Stochastic Low-frequency Variability in Three-dimensional Radiation Hydrodynamical Models of Massive Star Envelopes. , keywords =. doi:10.3847/2041-8213/ac441f , archivePrefix =. 2110.13944 , primaryClass =

    arXiv

  154. [163]

    Fundamental parameters and chemical abundances

    A volume-limited survey of mCP stars within 100 pc - I. Fundamental parameters and chemical abundances. , keywords =. doi:10.1093/mnras/sty3105 , archivePrefix =. 1811.05633 , primaryClass =

    arXiv

  155. [164]

    The IACOB project. I. Rotational velocities in northern Galactic O- and early B-type stars revisited. The impact of other sources of line-broadening. , keywords =. doi:10.1051/0004-6361/201322758 , archivePrefix =. 1311.3360 , primaryClass =

    arXiv

  156. [165]

    The IACOB project . III. New observational clues to understand macroturbulent broadening in massive O- and B-type stars. , keywords =. doi:10.1051/0004-6361/201628541 , archivePrefix =. 1608.05508 , primaryClass =

    arXiv

  157. [166]

    Hunting for spectroscopic binaries in the O and B supergiant domain.The threat of pulsational variability

    The IACOB project: CVIII. Hunting for spectroscopic binaries in the O and B supergiant domain.The threat of pulsational variability. arXiv e-prints , keywords =. doi:10.48550/arXiv.2405.11209 , archivePrefix =. 2405.11209 , primaryClass =

    doi arXiv

  158. [167]

    , keywords =

    Chemically Peculiar Hot Stars. , keywords =. doi:10.1007/BF02424427 , adsurl =

    doi

  159. [168]

    , keywords =

    High-mass pulsators in eclipsing binaries observed using TESS. , keywords =. doi:10.1093/mnras/stac875 , archivePrefix =. 2203.15365 , primaryClass =

    arXiv

  160. [169]

    , keywords =

    Discovery of Cep pulsations in the eclipsing binary V453 Cygni. , keywords =. doi:10.1093/mnrasl/slaa091 , archivePrefix =. 2005.07559 , primaryClass =

    2005 arXiv

  161. [170]

    arXiv e-prints , keywords =

    Pulsations in Binary Star Systems. arXiv e-prints , keywords =. doi:10.48550/arXiv.2509.08426 , archivePrefix =. 2509.08426 , primaryClass =

    doi arXiv

  162. [171]

    A main-sequence magnetic, rotational, and magnetospheric biography

    The magnetic early B-type stars - III. A main-sequence magnetic, rotational, and magnetospheric biography. , keywords =. doi:10.1093/mnras/stz2551 , archivePrefix =. 1909.02530 , primaryClass =

    1909 arXiv

  163. [172]

    , keywords =

    Catalog of Galactic Cephei Stars. , keywords =. doi:10.1086/429408 , archivePrefix =. astro-ph/0506495 , primaryClass =

    arXiv

  164. [173]

    , year = 1950, month = jan, volume =

    A study of the spectrum and magnetic variable star HD 125248. , year = 1950, month = jan, volume =. doi:10.1093/mnras/110.4.395 , adsurl =

    1950 doi

  165. [174]

    , keywords =

    Spectrophotometric analysis of the 5200 A region for peculiar and normal stars. , keywords =. doi:10.1051/0004-6361/201322300 , archivePrefix =. 1402.1021 , primaryClass =

    arXiv

  166. [175]

    , keywords =

    SUPPNet: Neural network for stellar spectrum normalisation. , keywords =. doi:10.1051/0004-6361/202141480 , archivePrefix =. 2111.15052 , primaryClass =

    arXiv

  167. [176]

    , keywords =

    Domains of pulsational instability of low-frequency modes in rotating upper main sequence stars. , keywords =. doi:10.1093/mnras/stx738 , archivePrefix =. 1703.08075 , primaryClass =

    arXiv

  168. [177]

    , keywords =

    Convective-core overshooting and the final fate of massive stars. , keywords =. doi:10.1051/0004-6361/202347434 , archivePrefix =. 2311.05701 , primaryClass =

    arXiv

  169. [178]

    Convective excitation and spectra of internal gravity waves

    3D hydrodynamic simulations of massive main-sequence stars - II. Convective excitation and spectra of internal gravity waves. , keywords =. doi:10.1093/mnras/stae1162 , archivePrefix =. 2303.06125 , primaryClass =

    arXiv

  170. [179]

    , keywords =

    Magnetism in LAMOST CP stars observed by TESS. , keywords =. doi:10.1051/0004-6361/202450651 , archivePrefix =. 2406.11554 , primaryClass =

    arXiv

  171. [180]

    , keywords =

    Discovery of new magnetic Scuti stars and the impact of magnetism on pulsation excitation. , keywords =. doi:10.1051/0004-6361/202556757 , archivePrefix =. 2510.12341 , primaryClass =

  172. [181]

    , keywords =

    Kappa-mechanism excitation of retrograde mixed modes in rotating B-type stars. , keywords =. doi:10.1111/j.1365-2966.2005.09585.x , archivePrefix =. astro-ph/0506580 , primaryClass =

    2005

  173. [182]

    , keywords =

    GYRE: an open-source stellar oscillation code based on a new Magnus Multiple Shooting scheme. , keywords =. doi:10.1093/mnras/stt1533 , archivePrefix =. 1308.2965 , primaryClass =

    arXiv

  174. [183]

    , keywords =

    Angular momentum transport by heat-driven g-modes in slowly pulsating B stars. , keywords =. doi:10.1093/mnras/stx3142 , archivePrefix =. 1712.02420 , primaryClass =

    arXiv

  175. [184]

    , keywords =

    Interior rotation modelling of the Cep pulsator HD 192575 including multiplet asymmetries. , keywords =. doi:10.1051/0004-6361/202452885 , archivePrefix =. 2506.19948 , primaryClass =

    arXiv

  176. [185]

    , keywords =

    Binarity at LOw Metallicity (BLOeM): Enhanced multiplicity of early B-type dwarfs and giants at Z = 0.2 Z _. , keywords =. doi:10.1051/0004-6361/202453166 , archivePrefix =. 2503.21936 , primaryClass =

    arXiv

  177. [186]

    , keywords =

    Mass-loss predictions for O and B stars as a function of metallicity. , keywords =. doi:10.1051/0004-6361:20010127 , archivePrefix =. astro-ph/0101509 , primaryClass =

    arXiv

  178. [187]

    , keywords =

    Identification of New Classical Be Stars from the LAMOST Medium Resolution Survey. , keywords =. doi:10.3847/1538-4365/ac617a , archivePrefix =. 2203.15289 , primaryClass =

    arXiv

  179. [188]

    The CDS reference database for astronomical objects

    The SIMBAD astronomical database. The CDS reference database for astronomical objects. , keywords =. doi:10.1051/aas:2000332 , archivePrefix =. astro-ph/0002110 , primaryClass =

    arXiv

  180. [189]

    , keywords =

    The impact of initial mass dependent convective boundary mixing on the structure and fates of massive stars. , keywords =. doi:10.1093/mnras/staf2245 , archivePrefix =. 2512.11728 , primaryClass =

  181. [190]

    Stellar labels for hot stars from low-resolution spectra. I. The HotPayne method and results for 330 000 stars from LAMOST DR6. , keywords =. doi:10.1051/0004-6361/202141570 , archivePrefix =. 2108.02878 , primaryClass =

    arXiv

  182. [191]

    , keywords =

    The demographics of binary companions to stripped-envelope supernovae: confronting population synthesis models with observations. , keywords =. doi:10.1093/mnras/staf2208 , archivePrefix =. 2508.12677 , primaryClass =

  183. [192]

    RAA , year = 2012, month = jul, volume =

    LAMOST spectral survey An overview. RAA , year = 2012, month = jul, volume =. doi:10.1088/1674-4527/12/7/002 , adsurl =

    2012 doi

  184. [193]

    Multi-order TODCOR: Application to observations taken with the CORALIE echelle spectrograph. I. The system <ASTROBJ>HD 41004</ASTROBJ>. , keywords =. doi:10.1051/0004-6361:20030499 , archivePrefix =. astro-ph/0303055 , primaryClass =

    arXiv

  185. [194]

    and Haberland, Matt and Reddy, Tyler and Cournapeau, David and Burovski, Evgeni and Peterson, Pearu and Weckesser, Warren and Bright, Jonathan and

    Virtanen, Pauli and Gommers, Ralf and Oliphant, Travis E. and Haberland, Matt and Reddy, Tyler and Cournapeau, David and Burovski, Evgeni and Peterson, Pearu and Weckesser, Warren and Bright, Jonathan and. Nature Methods , year =

  186. [195]

    arXiv , Author =:1307.6212 , Journal =

    doi:10.1051/0004-6361/201322068 , Eid =. arXiv , Author =:1307.6212 , Journal =

    arXiv

  187. [196]

    , keywords =

    The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package. , keywords =. doi:10.3847/1538-4357/ac7c74 , archivePrefix =. 2206.14220 , primaryClass =

    arXiv

  188. [197]

    Harris and K

    Charles R. Harris and K. Jarrod Millman and St. Array programming with. 2020 , month = sep, journal =. doi:10.1038/s41586-020-2649-2 , publisher =

    2020 doi

  189. [198]

    Hunter, J. D. , Title =. Computing in Science & Engineering , Volume =

  190. [199]

    Communications in Asteroseismology , year = 2005, month = jun, volume =

    Period04 User Guide. Communications in Asteroseismology , year = 2005, month = jun, volume =. doi:10.1553/cia146s53 , adsurl =

    2005 doi

  191. [200]

    , keywords =

    The MiMeS survey of magnetism in massive stars: introduction and overview. , keywords =. doi:10.1093/mnras/stv2568 , archivePrefix =. 1511.08425 , primaryClass =

    arXiv

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