pith. sign in

arxiv: 2606.27278 · v1 · pith:2F6OZLSXnew · submitted 2026-06-25 · 🌌 astro-ph.SR · astro-ph.EP

Astrochemical Study of Early Embedded Disks

Eleonora Bianchi This is my paper

Pith reviewed 2026-06-26 02:48 UTC · model grok-4.3

classification 🌌 astro-ph.SR astro-ph.EP
keywords astrochemistryprotostellar disksmachine learningdata miningplanet formationexoplanetsmolecular abundancesdisk mass
0
0 comments X

The pith

The iSEEDs project integrates machine learning and data mining with astrochemistry to extract physical conditions and molecular abundances from protostellar disk datasets.

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

The paper identifies the lack of measurements for the mass and chemical composition of young protostellar disks as a barrier to comparing them with exoplanet populations. It introduces the iSEEDs project to address this by combining machine learning and data mining techniques with astrochemistry. The goal is to systematically pull out hidden physical conditions and molecular abundances from high-resolution observations of these early embedded environments. A sympathetic reader would see this as a practical route to linking disk properties directly to the outcomes of planet formation. Success would support analysis of data from missions that inventory exoplanet masses and compositions.

Core claim

The central claim is that building the iSEEDs framework, which merges machine learning and data mining with astrochemistry, supplies a robust method to extract the physical conditions and molecular abundances contained in high-resolution datasets of protostellar environments, thereby enabling meaningful comparisons between young disks and observed exoplanet populations.

What carries the argument

The iSEEDs project, a framework that integrates machine learning and data mining with astrochemistry to analyze high-resolution protostellar datasets.

If this is right

  • Systematic extraction of disk masses and chemical compositions from high-resolution data becomes feasible.
  • Direct comparisons between protostellar disk properties and exoplanet populations can be performed.
  • Data from missions such as Ariel can be interpreted in the context of formation conditions.
  • New research directions open for the study of young planet-forming disks.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • The same integration approach could be tested on other classes of astrophysical observations that face similar data-volume challenges.
  • Successful extraction might reveal chemical pathways that connect disk composition to the final makeup of planets.
  • Validation would require side-by-side tests against traditional astrochemistry models on benchmark datasets.

Load-bearing premise

Machine learning and data mining techniques, when combined with astrochemistry, will be sufficient to overcome current observational challenges in measuring disk mass and composition.

What would settle it

Apply the iSEEDs framework to an existing high-resolution dataset of a known protostellar disk and compare the derived mass and molecular abundances against independent measurements obtained through conventional modeling; a mismatch would falsify the claim that the integration reliably extracts the quantities.

Figures

Figures reproduced from arXiv: 2606.27278 by Eleonora Bianchi.

Figure 1
Figure 1. Figure 1: Schematic of a Sun-like star and planet formation, showing the transition from a prestellar core to a planetary system. This figure was generated using Gemini (Google) based on an original conceptual sketch provided by the author. 1.2 Young planet-forming disks In recent years, the advent of the ALMA interferometer has fundamentally challenged established frameworks of planet formation. More specifically, … view at source ↗
Figure 2
Figure 2. Figure 2: The "Astrochemical Study of Early Embedded Disks" (iSEEDs) project employs an interdisciplinary approach, integrating astrochemistry and data science to characterise the mass, chemical composition, and dust properties of a statistically significant sample of young planet-forming disks. Image credits: logo from the Italian Ministry of University and Research; project illustration designed by L. Giani; scien… view at source ↗
read the original abstract

The question of how our planet was formed and, more generally, how a planetary system forms is fundamental and has been addressed in a broad range of research domains. However, we still lack a comprehensive understanding of the basic aspects of the process of star and planet formation. In particular, the challenge of measuring the mass and chemical composition of young protostellar disks has, so far, hampered a meaningful comparison with observed exoplanet populations. This will become critical in the near future to interpret the results of European space missions, such as Ariel, which will yield a comprehensive inventory of exoplanetary masses and chemical compositions. Building on recent developments in astrochemistry and data science, this perspective explores future research avenues for the study of young planet-forming disks and introduces the project "Astrochemical Study of Early Embedded Disks" (iSEEDs). By integrating machine learning and data mining with astrochemistry, iSEEDs provides a robust framework to systematically extract the physical conditions and molecular abundances hidden within high-resolution datasets of protostellar environments.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

0 major / 0 minor

Summary. This perspective manuscript identifies challenges in measuring the mass and chemical composition of young protostellar disks, notes the upcoming relevance of missions such as Ariel for exoplanet comparisons, and introduces the iSEEDs project as an intended integration of machine learning, data mining, and astrochemistry to extract physical conditions and molecular abundances from high-resolution protostellar datasets.

Significance. If realized, the proposed data-driven approach could help address observational limitations in early disk studies and support cross-comparisons with exoplanet populations. The manuscript offers no completed derivations, datasets, code, or validation, so its value is as a high-level outline of future research directions rather than a demonstration of new capabilities.

Simulated Author's Rebuttal

0 responses · 0 unresolved

We thank the referee for their supportive review, recognition of the manuscript's scope as a high-level perspective on future research directions, and recommendation to accept. The iSEEDs project is presented as an outline of intended integration of machine learning with astrochemistry rather than a completed demonstration.

Circularity Check

0 steps flagged

No circularity; high-level perspective without derivations or fitted claims

full rationale

The paper is a perspective piece introducing the iSEEDs project. It states an intended integration of ML/data mining with astrochemistry but presents no equations, fitted parameters, predictions, or load-bearing derivations. The central claim is prospective and does not reduce to its own inputs by construction. No self-citations or ansatzes are invoked in a manner that creates circularity. This is the expected outcome for a non-quantitative project description.

Axiom & Free-Parameter Ledger

0 free parameters · 0 axioms · 0 invented entities

The paper is a perspective piece with no mathematical derivations, data fits, or new physical models; no free parameters, axioms, or invented entities are introduced.

pith-pipeline@v0.9.1-grok · 5703 in / 1097 out tokens · 38358 ms · 2026-06-26T02:48:27.028416+00:00 · methodology

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Reference graph

Works this paper leans on

225 extracted references · 212 canonical work pages · 51 internal anchors

  1. [1]

    , keywords =

    Chemical Variation among Protostellar Cores: Dependence on Prestellar Core Conditions. , keywords =. doi:10.3847/1538-4357/ab994a , archivePrefix =. 2006.11696 , primaryClass =

    work page doi:10.3847/1538-4357/ab994a 2006

  2. [2]

    The Astrophysical Journall , author =

    The 2014 ALMA Long Baseline Campaign: First Results from High Angular Resolution Observations toward the HL Tau Region. , keywords =. doi:10.1088/2041-8205/808/1/L3 , archivePrefix =. 1503.02649 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/2041-8205/808/1/l3 2014

  3. [3]

    ALminer: ALMA archive mining and visualization toolkit

  4. [4]

    Science , keywords =

    Gas flow and accretion via spiral streamers and circumstellar disks in a young binary protostar. Science , keywords =. doi:10.1126/science.aaw3491 , archivePrefix =. 1910.01141 , primaryClass =

    work page doi:10.1126/science.aaw3491 1910

  5. [5]

    Alves and L

    Felipe O. Alves and L. Ilsedore Cleeves and Josep M. Girart and Zhaohuan Zhu and Gabriel A. P. Franco and Alice Zurlo and Paola Caselli , title =. The Astrophysical Journal Letters , abstract =. 2020 , month =. doi:10.3847/2041-8213/abc550 , url =

    work page doi:10.3847/2041-8213/abc550 2020

  6. [6]

    , keywords =

    Submillimeter Continuum Observations of rho Ophiuchi A: The Candidate Protostar VLA 1623 and Prestellar Clumps. , keywords =. doi:10.1086/172425 , adsurl =

    work page doi:10.1086/172425

  7. [7]

    From Filamentary Networks to Dense Cores in Molecular Clouds: Toward a New Paradigm for Star Formation

    From Filamentary Networks to Dense Cores in Molecular Clouds: Toward a New Paradigm for Star Formation. Protostars and Planets VI , year = 2014, editor =. doi:10.2458/azu_uapress_9780816531240-ch002 , archivePrefix =. 1312.6232 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.2458/azu_uapress_9780816531240-ch002 2014

  8. [8]

    Radio Jets from Young Stellar Objects

    Radio jets from young stellar objects. , keywords =. doi:10.1007/s00159-018-0107-z , archivePrefix =. 1806.06444 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1007/s00159-018-0107-z

  9. [9]

    , keywords =

    Physical properties of accretion shocks toward the Class I protostellar system Oph-IRS 44. , keywords =. doi:10.1051/0004-6361/202244312 , archivePrefix =. 2209.02827 , primaryClass =

    work page doi:10.1051/0004-6361/202244312

  10. [10]

    The Perseus ALMA Chemical Survey (PEACHES). III. Sulfur-bearing species tracing accretion and ejection processes in young protostars. , keywords =. doi:10.1051/0004-6361/202346728 , archivePrefix =. 2309.05839 , primaryClass =

    work page doi:10.1051/0004-6361/202346728

  11. [11]

    Early Planet Formation in Embedded Disks (eDisk). VI. Kinematic Structures around the Very-low-mass Protostar IRAS 16253-2429. , keywords =. doi:10.3847/1538-4357/ace624 , archivePrefix =. 2309.01891 , primaryClass =

    work page doi:10.3847/1538-4357/ace624

  12. [12]

    , keywords =

    Grain Size in the Class I Protostellar System TMC-1A Constrained with ALMA and Very Large Array Observations. , keywords =. doi:10.3847/1538-4357/ad938e , archivePrefix =. 2411.13044 , primaryClass =

    work page doi:10.3847/1538-4357/ad938e

  13. [13]

    Protostars and Planets VII , year = 2023, editor =

    Structured Distributions of Gas and Solids in Protoplanetary Disks. Protostars and Planets VII , year = 2023, editor =. doi:10.48550/arXiv.2210.13314 , archivePrefix =. 2210.13314 , primaryClass =

    work page doi:10.48550/arxiv.2210.13314 2023

  14. [14]

    Ball and Robert J

    Nicholas M. Ball and Robert J. Brunner and Adam D. Myers and David Tcheng , title =. The Astrophysical Journal , abstract =. 2006 , month =. doi:10.1086/507440 , url =

    work page doi:10.1086/507440 2006

  15. [15]

    Protostars and Planets V , year = 2007, editor =

    Observations of Jets and Outflows from Young Stars. Protostars and Planets V , year = 2007, editor =

    2007

  16. [16]

    , year = 2025, month = may, volume =

    Gaseous methanol in cold environments: is thermal desorption from low binding energy sites the explanation?. , year = 2025, month = may, volume =. doi:10.1093/mnras/staf476 , adsurl =

    work page doi:10.1093/mnras/staf476 2025

  17. [17]

    On the diversity and statistical properties of protostellar discs

    On the diversity and statistical properties of protostellar discs. , keywords =. doi:10.1093/mnras/sty169 , archivePrefix =. 1801.07721 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1093/mnras/sty169

  18. [18]

    , keywords =

    Questioning the spatial origin of complex organic molecules in young protostars with the CALYPSO survey. , keywords =. doi:10.1051/0004-6361/201937352 , archivePrefix =. 2002.00592 , primaryClass =

    work page doi:10.1051/0004-6361/201937352 2002

  19. [19]

    , keywords =

    A Circumplanetary Disk around PDS70c. , keywords =. doi:10.3847/2041-8213/ac0f83 , archivePrefix =. 2108.07123 , primaryClass =

    work page doi:10.3847/2041-8213/ac0f83 2041

  20. [20]

    , keywords =

    Cold Dark Clouds: The Initial Conditions for Star Formation. , keywords =. doi:10.1146/annurev.astro.45.071206.100404 , archivePrefix =. 0705.3765 , primaryClass =

    work page doi:10.1146/annurev.astro.45.071206.100404

  21. [21]

    Decrease of the organic deuteration during the evolution of Sun-like protostars: the case of SVS13-A

    Decrease of the organic deuteration during the evolution of Sun-like protostars: the case of SVS13-A. , keywords =. doi:10.1093/mnras/stx252 , archivePrefix =. 1701.08656 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1093/mnras/stx252

  22. [22]

    Deuterated methanol on Solar System scale around the HH212 protostar

    Deuterated methanol on a solar system scale around the HH212 protostar. , keywords =. doi:10.1051/0004-6361/201731404 , archivePrefix =. 1709.04726 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1051/0004-6361/201731404

  23. [23]

    The hot corino at the heart of the prototypical Class I protostar L1551 IRS5

    FAUST I. The hot corino at the heart of the prototypical Class I protostar L1551 IRS5. , keywords =. doi:10.1093/mnrasl/slaa130 , archivePrefix =. 2007.10275 , primaryClass =

    work page doi:10.1093/mnrasl/slaa130 2007

  24. [24]

    SOLIS. XV. CH _ 3 CN deuteration in the SVS13-A Class I hot corino. , keywords =. doi:10.1051/0004-6361/202141893 , adsurl =

    work page doi:10.1051/0004-6361/202141893

  25. [25]

    , keywords =

    The Two Hot Corinos of the SVS13-A Protostellar Binary System: Counterposed Siblings. , keywords =. doi:10.3847/2041-8213/ac5a56 , archivePrefix =. 2203.03412 , primaryClass =

    work page doi:10.3847/2041-8213/ac5a56 2041

  26. [26]

    Faraday Discussions , keywords =

    Streamers feeding the SVS13-A protobinary system: astrochemistry reveals accretion shocks?. Faraday Discussions , keywords =. doi:10.1039/D3FD00018D , archivePrefix =. 2306.08539 , primaryClass =

    work page doi:10.1039/d3fd00018d

  27. [27]

    , keywords =

    Cyanopolyyne Chemistry in the L1544 Prestellar Core: New Insights from GBT Observations. , keywords =. doi:10.3847/1538-4357/acb5e8 , archivePrefix =. 2301.10106 , primaryClass =

    work page doi:10.3847/1538-4357/acb5e8

  28. [28]

    arXiv e-prints , keywords =

    Molecular complexity of young solar analogues. arXiv e-prints , keywords =. doi:10.48550/arXiv.2407.10882 , archivePrefix =. 2407.10882 , primaryClass =

    work page doi:10.48550/arxiv.2407.10882

  29. [29]

    , keywords =

    Birnstiel, Tilman. Dust Growth and Evolution in Protoplanetary Disks. Annual Review of Astronomy and Astrophysics. 2024. doi:https://doi.org/10.1146/annurev-astro-071221-052705

    work page doi:10.1146/annurev-astro-071221-052705 2024

  30. [30]

    , keywords =

    Was Earth's Water Acquired Locally during the Earliest Phases of the Solar System Formation?. , keywords =. doi:10.3847/2041-8213/ade5aa , archivePrefix =. 2507.03968 , primaryClass =

    work page doi:10.3847/2041-8213/ade5aa 2041

  31. [31]

    Astrochemical Inheritance of Terrestrial Planets Water from Local Wet Silicates

    Astrochemical inheritance of terrestrial planets water from local wet silicates. , keywords =. doi:10.1093/mnras/stag789 , archivePrefix =. 2605.02637 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1093/mnras/stag789

  32. [32]

    Complex molecules in the hot core of the low mass protostar NGC1333-IRAS4A

    Complex Molecules in the Hot Core of the Low-Mass Protostar NGC 1333 IRAS 4A. , keywords =. doi:10.1086/423952 , archivePrefix =. astro-ph/0407154 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1086/423952

  33. [33]

    , keywords =

    Hunting for hot corinos and WCCC sources in the OMC-2/3 filament. , keywords =. doi:10.1051/0004-6361/201937164 , archivePrefix =. 2003.06198 , primaryClass =

    work page doi:10.1051/0004-6361/201937164 2003

  34. [34]

    ORion Alma New GEneration Survey (ORANGES). I. Dust continuum and free-free emission of OMC-2/3 filament protostars. , keywords =. doi:10.1051/0004-6361/202141157 , archivePrefix =. 2107.10743 , primaryClass =

    work page doi:10.1051/0004-6361/202141157

  35. [35]

    , keywords =

    The Chemical Nature of Orion Protostars: Are ORANGES Different from PEACHES? ORANGES II. , keywords =. doi:10.3847/1538-4357/ac5904 , archivePrefix =. 2202.13835 , primaryClass =

    work page doi:10.3847/1538-4357/ac5904

  36. [36]

    ALMA dual-band constraints on grain properties and the mass-infall rate

    A dusty streamer infalling onto the disk of a class I protostar. ALMA dual-band constraints on grain properties and the mass-infall rate. , keywords =. doi:10.1051/0004-6361/202347486 , archivePrefix =. 2311.13723 , primaryClass =

    work page doi:10.1051/0004-6361/202347486

  37. [37]

    The dust opacity spectral indices of protostellar envelopes bridge the gap between interstellar medium and disks

    FAUST: XXVI. The dust opacity spectral indices of protostellar envelopes bridge the gap between interstellar medium and disks. , keywords =. doi:10.1051/0004-6361/202554645 , archivePrefix =. 2506.06865 , primaryClass =

    work page doi:10.1051/0004-6361/202554645

  38. [38]

    , keywords =

    Anatomy of a fall: stationary and super-Keplerian spiral arms generated by accretion streamers in protostellar discs. , keywords =. doi:10.1093/mnras/staf135 , archivePrefix =. 2410.18521 , primaryClass =

    work page doi:10.1093/mnras/staf135

  39. [39]

    arXiv e-prints , keywords =

    Inferring stellar parameters and their uncertainties from high-resolution spectroscopy using invertible neural networks. arXiv e-prints , keywords =. doi:10.48550/arXiv.2409.10621 , archivePrefix =. 2409.10621 , primaryClass =

    work page doi:10.48550/arxiv.2409.10621

  40. [40]

    arXiv e-prints , keywords =

    The ALMA Development Program: Roadmap to 2030. arXiv e-prints , keywords =. doi:10.48550/arXiv.2001.11076 , archivePrefix =. 2001.11076 , primaryClass =

    work page doi:10.48550/arxiv.2001.11076 2030

  41. [41]

    , keywords =

    The Radial Distribution of Dust Particles in the HL Tau Disk from ALMA and VLA Observations. , keywords =. doi:10.3847/1538-4357/ab3d33 , archivePrefix =. 1908.07140 , primaryClass =

    work page doi:10.3847/1538-4357/ab3d33 1908

  42. [42]

    Our astrochemical heritage

    Our astrochemical heritage. , keywords =. doi:10.1007/s00159-012-0056-x , archivePrefix =. 1210.6368 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1007/s00159-012-0056-x

  43. [43]

    , keywords =

    The Hot Core around the Low-mass Protostar IRAS 16293-2422: Scoundrels Rule!. , keywords =. doi:10.1086/378038 , adsurl =

    work page doi:10.1086/378038

  44. [44]

    , year = 2000, month = may, volume =

    The hot core of the solar-type protostar IRAS 16293-2422: H\_2CO emission. , year = 2000, month = may, volume =

    2000

  45. [45]

    Theoretical HDO emission from low-mass protostellar envelopes

    Theoretical H _ 2 CO emission from protostellar envelopes. , keywords =. doi:10.1051/0004-6361:20031243 , archivePrefix =. astro-ph/0506144 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1051/0004-6361:20031243

  46. [46]

    Star Formation in the Interstellar Medium: In Honor of David Hollenbach , year = 2004, editor =

    The Hot Corinos of Solar Type Protostars. Star Formation in the Interstellar Medium: In Honor of David Hollenbach , year = 2004, editor =

    2004

  47. [47]

    Deuterium Fractionation: the Ariadne's Thread from the Pre-collapse Phase to Meteorites and Comets today

    Deuterium Fractionation: The Ariadne's Thread from the Precollapse Phase to Meteorites and Comets Today. Protostars and Planets VI , year = 2014, editor =. doi:10.2458/azu_uapress_9780816531240-ch037 , archivePrefix =. 1403.7143 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.2458/azu_uapress_9780816531240-ch037 2014

  48. [48]

    Seeds Of Life In Space (SOLIS): The organic composition diversity at 300--1000 au scale in Solar-type star forming regions

    Seeds Of Life In Space (SOLIS): The Organic Composition Diversity at 300-1000 au Scale in Solar-type Star-forming Regions. , keywords =. doi:10.3847/1538-4357/aa961d , archivePrefix =. 1710.10437 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.3847/1538-4357/aa961d

  49. [49]

    Protostars and Planets VII , year = 2023, editor =

    Organic Chemistry in the First Phases of Solar-Type Protostars. Protostars and Planets VII , year = 2023, editor =

    2023

  50. [50]

    , keywords =

    Pure hydrocarbon cycles in TMC-1: Discovery of ethynyl cyclopropenylidene, cyclopentadiene, and indene. , keywords =. doi:10.1051/0004-6361/202141156 , archivePrefix =. 2104.13991 , primaryClass =

    work page doi:10.1051/0004-6361/202141156

  51. [51]

    , keywords =

    Chemically Fresh Gas Inflows Detected in a Nearby High-mass Star-forming Region. , keywords =. doi:10.3847/2041-8213/ac3ec8 , adsurl =

    work page doi:10.3847/2041-8213/ac3ec8 2041

  52. [52]

    Protostar L1455 IRS1: Rotating Disk Connecting to Filamentary Network

    Protostar L1455 IRS1: A Rotating Disk Connecting to a Filamentary Network. , keywords =. doi:10.3847/0004-637X/823/2/151 , archivePrefix =. 1512.07756 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.3847/0004-637x/823/2/151

  53. [53]

    Seeds of Life in Space (SOLIS). II. Formamide in protostellar shocks: Evidence for gas-phase formation. , keywords =. doi:10.1051/0004-6361/201731249 , archivePrefix =. 1708.04663 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1051/0004-6361/201731249

  54. [54]

    Water and interstellar complex organics associated with the HH 212 protostellar disc - On disc atmospheres, disc winds, and accretion shocks

    Water and interstellar complex organics associated with the HH 212 protostellar disc. On disc atmospheres, disc winds, and accretion shocks. , keywords =. doi:10.1051/0004-6361/201832765 , archivePrefix =. 1806.07967 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1051/0004-6361/201832765

  55. [55]

    Frontiers in Astronomy and Space Sciences , keywords =

    Enlightening the chemistry of infalling envelopes and accretion disks around Sun-like protostars: the ALMA FAUST project. Frontiers in Astronomy and Space Sciences , keywords =. doi:10.3389/fspas.2021.782006 , archivePrefix =. 2111.14121 , primaryClass =

    work page doi:10.3389/fspas.2021.782006 2021

  56. [56]

    Accretion streamers and jets in the VLA 1623-2417 protocluster

    FAUST XII. Accretion streamers and jets in the VLA 1623-2417 protocluster. , keywords =. doi:10.1093/mnras/stae472 , archivePrefix =. 2402.10258 , primaryClass =

    work page doi:10.1093/mnras/stae472

  57. [57]

    European Physical Journal Plus , keywords =

    Close encounters: How stellar flybys shape planet-forming discs. European Physical Journal Plus , keywords =. doi:10.1140/epjp/s13360-022-03602-w , archivePrefix =. 2207.09752 , primaryClass =

    work page doi:10.1140/epjp/s13360-022-03602-w

  58. [58]

    , keywords =

    Population synthesis models indicate a need for early and ubiquitous disk substructures. , keywords =. doi:10.1051/0004-6361/202450328 , archivePrefix =. 2405.14501 , primaryClass =

    work page doi:10.1051/0004-6361/202450328

  59. [59]

    , keywords =

    Hot Corinos Chemical Diversity: Myth or Reality?. , keywords =. doi:10.3847/2041-8213/ab8d41 , archivePrefix =. 2006.04484 , primaryClass =

    work page doi:10.3847/2041-8213/ab8d41 2041

  60. [60]

    Protostars and Planets VII , year = 2023, editor =

    Planet Formation Theory in the Era of ALMA and Kepler: from Pebbles to Exoplanets. Protostars and Planets VII , year = 2023, editor =. doi:10.48550/arXiv.2203.09759 , archivePrefix =. 2203.09759 , primaryClass =

    work page doi:10.48550/arxiv.2203.09759 2023

  61. [61]

    RADMC-3D: A multi-purpose radiative transfer tool

  62. [62]

    Young Stellar Objects in the Gould Belt

    Young Stellar Objects in the Gould Belt. , keywords =. doi:10.1088/0067-0049/220/1/11 , archivePrefix =. 1508.03199 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/0067-0049/220/1/11

  63. [63]

    , keywords =

    Sulfur monoxide (SO) as a shock tracer in protoplanetary disks: Case of AB Aurigae. , keywords =. doi:10.1051/0004-6361/202451299 , archivePrefix =. 2408.14276 , primaryClass =

    work page doi:10.1051/0004-6361/202451299

  64. [64]

    ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP). II. Survey Overview: A First Look at 1.3 mm Continuum Maps and Molecular Outflows. , keywords =. doi:10.3847/1538-4365/abba26 , archivePrefix =. 2010.14507 , primaryClass =

    work page doi:10.3847/1538-4365/abba26 2010

  65. [65]

    , keywords =

    The Chemical Inventory of the Planet-hosting Disk PDS 70. , keywords =. doi:10.3847/1538-3881/abf0a4 , archivePrefix =. 2101.08369 , primaryClass =

    work page doi:10.3847/1538-3881/abf0a4

  66. [66]

    , keywords =

    Binding Energies of Interstellar Molecules on Crystalline and Amorphous Models of Water Ice by Ab Initio Calculations. , keywords =. doi:10.3847/1538-4357/abb953 , archivePrefix =. 2009.09763 , primaryClass =

    work page doi:10.3847/1538-4357/abb953 2009

  67. [67]

    , keywords =

    The Mass Accretion Rate and Stellar Properties in Class I Protostars. , keywords =. doi:10.3847/1538-4357/aca320 , archivePrefix =. 2211.07653 , primaryClass =

    work page doi:10.3847/1538-4357/aca320

  68. [68]

    Protostars and Planets VII , year = 2023, editor =

    Accretion Variability as a Guide to Stellar Mass Assembly. Protostars and Planets VII , year = 2023, editor =. doi:10.48550/arXiv.2203.11257 , archivePrefix =. 2203.11257 , primaryClass =

    work page doi:10.48550/arxiv.2203.11257 2023

  69. [69]

    Early Planet Formation in Embedded Disks (eDisk). XII. Accretion Streamers, Protoplanetary Disk, and Outflow in the Class I Source Oph IRS 63. , keywords =. doi:10.3847/1538-4357/acf7c1 , archivePrefix =. 2310.14617 , primaryClass =

    work page doi:10.3847/1538-4357/acf7c1

  70. [70]

    , keywords =

    The influence of grains on the propagation and structure of C-type shock waves in interstellar molecular clouds. , keywords =. doi:10.1046/j.1365-8711.2003.06716.x , adsurl =

    work page doi:10.1046/j.1365-8711.2003.06716.x 2003

  71. [71]

    Protostars and Planets VI , year = 2014, editor =

    Jets and Outflows from Star to Cloud: Observations Confront Theory. Protostars and Planets VI , year = 2014, editor =. doi:10.2458/azu_uapress_9780816531240-ch020 , archivePrefix =. 1402.3553 , primaryClass =

    work page doi:10.2458/azu_uapress_9780816531240-ch020 2014

  72. [72]

    The chemical structure and temperature profile of the IRAS 4A2 hot corino at 20 50 au

    FAUST: XX. The chemical structure and temperature profile of the IRAS 4A2 hot corino at 20-50 au. , keywords =. doi:10.1051/0004-6361/202452191 , archivePrefix =. 2501.19188 , primaryClass =

    work page doi:10.1051/0004-6361/202452191

  73. [73]

    The Herschel Orion Protostar Survey: Spectral Energy Distributions and Fits Using a Grid of Protostellar Models

    The Herschel Orion Protostar Survey: Spectral Energy Distributions and Fits Using a Grid of Protostellar Models. , keywords =. doi:10.3847/0067-0049/224/1/5 , archivePrefix =. 1602.07314 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.3847/0067-0049/224/1/5

  74. [74]

    , keywords =

    Low dust emissivities and radial variations in the envelopes of Class 0 protostars: possible signature of early grain growth. , keywords =. doi:10.1051/0004-6361/201936342 , archivePrefix =. 1910.04652 , primaryClass =

    work page doi:10.1051/0004-6361/201936342 1910

  75. [75]

    ALMA chemical survey of disk-outflow sources in Taurus (ALMA-DOT). V. Sample, overview, and demography of disk molecular emission. , keywords =. doi:10.1051/0004-6361/202039483 , archivePrefix =. 2012.07667 , primaryClass =

    work page doi:10.1051/0004-6361/202039483 2012

  76. [76]

    ALMA chemical survey of disk-outflow sources in Taurus (ALMA-DOT). VI. Accretion shocks in the disk of DG Tau and HL Tau. , keywords =. doi:10.1051/0004-6361/202141264 , archivePrefix =. 2110.13820 , primaryClass =

    work page doi:10.1051/0004-6361/202141264

  77. [77]

    , keywords =

    Revised gas-phase formation network of methyl cyanide: the origin of methyl cyanide and methanol abundance correlation in hot corinos. , keywords =. doi:10.1093/mnras/stad2892 , archivePrefix =. 2309.12745 , primaryClass =

    work page doi:10.1093/mnras/stad2892

  78. [78]

    , keywords =

    A comprehensive study of the gas-phase formation network of HC _ 5 N: theory, experiments, observations, and models. , keywords =. doi:10.1093/mnras/staf189 , archivePrefix =. 2502.03046 , primaryClass =

    work page doi:10.1093/mnras/staf189

  79. [79]

    Infalling streamers in L1448N

    ANTIHEROES-PRODIGE: Quantifying the connection from the envelope to the disk with the IRAM 30 m telescope and NOEMA: I. Infalling streamers in L1448N. , keywords =. doi:10.1051/0004-6361/202555688 , archivePrefix =. 2507.16303 , primaryClass =

    work page doi:10.1051/0004-6361/202555688

  80. [80]

    , keywords =

    Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): Late Infall Causing Disk Misalignment and Dynamic Structures in SU Aur. , keywords =. doi:10.3847/2041-8213/abdf57 , archivePrefix =. 2102.08781 , primaryClass =

    work page doi:10.3847/2041-8213/abdf57 2041

Showing first 80 references.