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| variable = [[Rapidly oscillating Ap star|roAp]]<ref name=sachkov/> ...ef name=csiro/> It is a type of [[chemically peculiar star]] known as an [[Ap star]], as indicated by the 'p' in the [[stellar classification]]. ...

...a Scuti variable]]s, [[SX Phoenicis variable]]s, and [[rapidly oscillating Ap star]]s (roAps) near the [[main sequence]]; [[RR Lyrae variables]] where it [[File:HR Diagram for pulsating stars.svg|thumb|left|[[HR diagram]] for [[pulsating star]]s]] ...

{{Short description|Study of oscillations in stars}} '''Asteroseismology''' is the study of oscillations in stars. Stars have many [[Resonance|resonant]] modes and frequencies, and the path of sou ...

| variable = [[Rapidly oscillating Ap star|roAp]]<ref name=gcvs/> This star belongs to a class of variables known as [[rapidly oscillating Ap stars]]. It oscillates with multiple, non-radial pulsation cycles and a dominant ...

| variable=[[rapidly oscillating Ap star|roAp]]<ref name=gcvs/><ref name=hubrig/> ...n |first3=A A |date=2018-11-01 |title=New catalogue of chemically peculiar stars, and statistical analysis |journal=Monthly Notices of the Royal Astronomica ...

......102025S|title=VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)|journal=VizieR On-line Data Catalog: B/GCVS. Originally ...&AS..130..223N|doi=10.1051/aas:1998365|title=Multiplicity among peculiar a stars|journal=Astronomy and Astrophysics Supplement Series|volume=130|issue=2|pag ...

...to have been formed from the merger of two [[white dwarf]]s. Two sun-like stars have planetary systems: [[HD 134060]] has two small planets, and [[HD 12944 ...rcinus lies adjacent to the [[Alpha Centauri|Alpha]] and [[Beta Centauri]] stars. As it is at [[declination]] −50° to −70°, the whole constellation is only ...

** [[Circumbinary planet]] – an exoplanet that orbits two stars. ...ve high surface temperatures because they orbit very close to their parent stars, whereas Jupiter orbits its parent star (the [[Sun]]) at 5.2&nbsp;AU (780×1 ...

...are multiple star systems with six and five components respectively. Five stars in the constellation host [[Jupiter]]-sized [[exoplanet]]s. [[Abell 2065]] ...he horizon to observers between the 50°S and [[64th parallel south|64°S]], stars within a few degrees of the horizon are to all intents and purposes unobser ...

...t=Alexeev |first=Boris V. |chapter=Chapter 7 - Nonlocal Theory of Variable Stars |date=2017-01-01 |chapter-url=https://www.sciencedirect.com/science/article ...ef>{{cite journal | title=Cross-matching the General Catalogue of Variable Stars with the Gaia DR3 source catalogue | display-authors=1 | last1=Ansari | fir ...

...url=|pmc=10995993 }}</ref> In another study, it was shown that in a model oscillating [[Hadean]] environment likely to have been abundant during early evolution, ...ite.com/article/20120829/DA0V31D80.html |date=August 29, 2012 |publisher=[[AP News]] |access-date=August 31, 2012 |url-status=live |archive-url=https://w ...

...ship between these parameters is expressed by the [[Lawson criterion]]. In stars, gravity provides the conditions for fusing [[hydrogen]] isotopes. Experime ...by generating the field using a non-neutral cloud. These include a plasma oscillating device,<ref>{{Cite journal|last1=Barnes|first1=D. C.|last2=Nebel|first2=R. ...