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...pa Pavonis TESS lightcurve.png|thumb|Lightcurve of the W Virginis (Type II Cepheid) variable κ Pavonis recorded by NASA's Transiting Exoplanet Survey Satellit '''W Virginis variables''' are a subclass of [[Type II Cepheid]]s which exhibit pulsation periods between 10–20 days,<ref name=wallerstein ...

| variable = [[Classical Cepheid]]<ref name=gcvs>{{cite journal|bibcode=2009yCat....102025S|title=VizieR Onl ...journal|bibcode= 2007A&A...476...73F|title= A new calibration of Galactic Cepheid period-luminosity relations from B to K bands, and a comparison to LMC rela ...

A '''Delta Scuti variable''' (sometimes termed '''dwarf cepheid''' when the V-band amplitude is larger than 0.3 mag.) is a class of [[pulsa ...The [[OGLE]] and [[MACHO]] surveys have detected nearly 3,000 Delta Scuti variables in the [[Large Magellanic Cloud]].<ref name=poleski2010/><ref name=garg2010 ...

| variable = [[Classical Cepheid variable|δ Cep]]<ref name=gcvs>{{cite journal|bibcode=2009yCat....102025S|t ...5|title=Hubble Space Telescope Fine Guidance Sensor Parallaxes of Galactic Cepheid Variable Stars: Period-Luminosity Relations|journal=The Astronomical Journa ...

|variable=[[Classical Cepheid variable|δ Cep]]<ref name=gcvs/> |dist_pc=473<ref name=cepheid/> ...

| variable = [[Classical Cepheid variable|Cepheid]]<ref name=gcvs/> ...[stellar classification]] of F7II.<ref name=houk1979/> It is a [[Classical Cepheid variable]] that ranges in [[apparent magnitude]] from 4.20 down to 4.90 wit ...

...many of the longest-known variable stars, including the [[Cepheid variable|Cepheid]] and [[RR Lyrae variable]]s. ...irst5 = Corinne | title = Driving the Gravity-Mode Pulsations in γ Doradus Variables | date = 10 October 2000 | journal = The Astrophysical Journal Letters | vo ...

Epsilon Leonis exhibits the characteristics of a [[Cepheid variable|Cepheid-like variable]], changing by an amplitude of 0.3 [[Magnitude (astronomy)|ma [[Category:Classical Cepheid variables]] ...

{{redirect|Cepheid|}} ...1243686232.jpg|thumb|upright=1.4|[[RS Puppis]], one of the brightest known Cepheid variable stars in the [[Milky Way]] galaxy<br />(<small>[[Hubble Space Tele ...

'''RR Lyrae variables''' are periodic [[variable star]]s, commonly found in [[globular clusters]] ...and reported by Pickering in 1900 as "indistinguishable from cluster-type variables".<ref name=smith2004/> ...

| variable = [[Classical Cepheid variable|Classical Cepheid]]<ref name=gcvs/> ...n [[Pollux (star)|Pollux]]. It is a [[classical Cepheid variable|classical Cepheid]] [[variable star]], of which over 800 have been found in our galaxy. As s ...

...scribed as a ''pseudo-Cepheid'', a supergiant with pulsations similar to a Cepheid but less regular.<ref name=usenko/> ...:1998129 |title=Hipparcos photometry of 24 variable massive stars (α Cygni variables) |journal=Astronomy and Astrophysics Supplement Series |volume=128 |pages=1 ...

| variable = [[Classical Cepheid variable|δ Cep]]<ref name=GCVS-eta-Aql/> ...|abbr=off|lk=on}}.<ref name="DR3"/> The primary component is a [[Classical Cepheid variable]].<ref name=GCVS-eta-Aql/> ...

...riable star type|Delta Cephei variable|the general class of variable stars|Cepheid variable}} | variable = [[Cepheid variable|Cepheid]] ...

...w:<ref name="NYT-20240327" /> the [[period-luminosity relation]]ship for [[Cepheid variable]]s ...r [[galaxy|galaxies]].<ref name="1777Variables">{{cite journal |title=1777 variables in the Magellanic Clouds |last=Leavitt |first=Henrietta S. |date=1908 |jour ...

...bility strip]] on the HR diagram where the majority of stars are pulsating variables. The instability strip reaches from the main sequence up to hypergiant lumi *[[W Virginis variable]]s, more-luminous pulsating variables also known as type II Cepheids, with periods of 10–20 days; ...

...|title=An international co-operation for the photographic study of Cepheid variables|journal=Popular Astronomy|volume=34|pages=493|last1=Henroteau|first1=F.|yea [[Classical Cepheid variables]] typically have supergiant luminosity classes, although only the most lumi ...

...d in the [[General Catalogue of Variable Stars]] as a possible [[Classical Cepheid variable|δ Cep variable]].<ref name=ibvs/> Further observations refined th [[Category:Cepheid variables]] ...

===Cepheid variables=== ...eid variable]] stars in 25&nbsp;galaxies. Theory suggests that the rate of cepheid pulsation in galaxies screened from a hypothetical fifth force by neighbour ...

...e than once and pulsate as [[Classical Cepheid variable|Type I (Classical) Cepheid variable]]s.<ref name=bono>{{cite journal|bibcode=2000ApJ...543..955B|arxiv ...ilson>{{cite journal|bibcode=2011A&A...529L...9N|arxiv=1104.1638|title=The Cepheid mass discrepancy and pulsation-driven mass loss|journal=Astronomy & Astroph ...