Pith. sign in

REVIEW 3 cited by

Delta Scuti Variables

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2110.09806 v1 pith:RHSU7R42 submitted 2021-10-19 astro-ph.SR

classification astro-ph.SR
keywords deltascutisomestarsvariablesasteroseismicbeforeindividual
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

We review recent research on Delta Scuti stars from an observer's viewpoint. First, some signposts helping to lead the way through the Delta Scuti jungle are placed. Then, some problems in studying individual pulsators in the framework of asteroseismology are given before a view on how the study of these variables has benefited (or not) from past and present high-precision asteroseismic space missions is presented. Some possible pitfalls in the analysis of data with a large dynamical range in pulsational amplitudes are pointed out, and a strategy to optimize the outcome of asteroseismic studies of Delta Scuti stars is suggested. We continue with some views on "hybrid" pulsators and interesting individual High Amplitude Delta Scuti stars, and then take a look on Delta Scuti stars in stellar systems of several different kinds. Recent results on pre-main sequence Delta Scuti stars are discussed as are questions related to the instability strip of these variables. Finally, some remarkable new theoretical results are highlighted before, instead of a set of classical conclusions, questions to be solved in the future, are raised.

Discussion (0). Sign in to comment.

Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. SRG/eROSITA X-ray selected cataclysmic variable candidates observed in SDSS-V DR20

    astro-ph.SR 2026-07 conditional novelty 6.0 of 10

    eROSITA-selected SDSS-V DR20 spectroscopy yields 587 cataclysmic variables (274 known), including new nearby systems, AM CVns, and a low-accretion-rate polar.

  2. The Longest-period Young Transiting Exoplanets. A Duo of Puffy Giants inside a Debris Disk

    astro-ph.EP 2026-07 conditional novelty 6.0 of 10

    HD 114082 hosts two puffy, moderate-to-low-mass giants on nearly circular, coplanar, near-resonant orbits of 225.55 and ~314 days, the longest-period young transiting exoplanets known.

  3. Precise Asteroseismology of the High-amplitude Delta Scuti Star EH Librae, an AE UMa Analogue in the Hertzsprung Gap

    astro-ph.SR 2025-07 conditional novelty 5.0 of 10

    EH Librae is a single-mode high-amplitude Delta Scuti star in the Hertzsprung gap; its period increase of 5.4 parts per billion per year is consistent with stellar evolution at a mass of 1.715 solar masses.

Pith tools