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...>|b-v=0.84<ref name=ucac4/>|u-b=-0.19<ref name=ucac4/>|variable=[[RV Tauri variable]]<ref name=manick/>}} ...sified as a B-type [[blue giant]], as well as being the hottest [[RV Tauri variable]] in the LMC. LHA 120-S 79 is also extremely luminous, at over 14,000 L☉,<r ...

{{Short description|Mira-type long period variable star in the constellation Corona Borealis}} ...date=4 January 2010|work=AAVSO Website|publisher=[[American Association of Variable Star Observers]]|access-date=13 November 2014}}</ref> ...

{{Short description|Variable star in the constellation Scutum}} |variable=[[Semiregular variable star|SRb]] ...

...= Late [[Blue supergiant star|O supergiant]] or candidate [[luminous blue variable|LBV]]<ref name=humphreys/> | variable = [[luminous blue variable|cLBV]]?<ref name=humphreys/> ...

| names = [[Variable star designation|SS]] Vir, [[Hipparcos catalogue|HIP]] 120212, [[Henry Drap ...n]]s.<ref>{{cite journal |title = Near-infrared observations of the carbon stars TU Geminorum and SS Virginis at milliarcsecond resolution |last1 = Richichi ...

{{Short description|Variable star in the constellation Fornax}} | variable=[[Mira variable|Mira]]<ref name=gcvs/> ...

| variable=[[Slow irregular variable|LB]]<ref name=gcvs/> ...last6=Gootkin|first6=Keyan|title=Short Term Variability of Evolved Massive Stars with TESS II: A New Class of Cool, Pulsating Supergiants|journal=The Astrop ...

| variable = [[Slow irregular variable|Lb]]?<ref name=cgcvs2007/> ...[[asymptotic giant branch]].<ref name=eggen1992/> It is a [[slow irregular variable]] type LB that can increase in magnitude up to 4.38.<ref name=cgcvs2007/><r ...

|variable=[[Pulsating variable]]<ref name="SIMBAD"/> ...Puppis''', also known as HD 54475, is a [[B-type star]] and a [[pulsating variable]] in the constellation of [[Puppis]].<ref name="SIMBAD">{{Cite simbad|D Pup ...

| variable = [[Semiregular variable|SRb]]<ref name=Samus2017/> ...amus2017/> is visible to the [[naked eye]] and one of the brightest carbon stars.<ref name=Streicher2009/> Based on [[stellar parallax|parallax]] measuremen ...

| name = [[Variable star designation|R Volantis]] ...d]] [[light curve]] for R Volantis, plotted from [[American Association of Variable Star Observers|AAVSO]] data<ref name="aavso"/> ...

| variable ...Rayet star|Wolf-Rayet star]], as well as being a candidate [[Luminous blue variable]], located 4,142 light years away in the constellation of [[Scorpius]]. The ...

{{Short description|Variable star in the constellation Hydra}} | variable = [[semiregular variable star|SRb]]<ref name=Samus2017/> ...

{{about|p² Leonis|other stars with this Bayer designation|p Leonis}} | variable = suspected<ref name=nsv/> ...

...haracter|type=[[Yellow hypergiant]]|class=A2Ia+<ref name=clark/>|b-v=|u-b=|variable=}} ...s is closer to {{solar mass|20}}, it may evolve through an [[Luminous blue variable|LBV]] stage and get slightly hotter before exploding in a type IIb supernov ...

| variable = ...Cha]], [[Cordoba Durchmusterung|CD]]−77° 454, [[Catalogues of Fundamental Stars|FK5]] 401, [[Henry Draper Catalogue|HD]] 92305, [[Hipparcos Catalogue|HIP]] ...

{{Short description|Variable star in the constellation Orion}} ...articular star|the type of variable stars named after this star|FU Orionis stars}} ...

| variable = [[slow irregular variable|LC]]<ref name=gcvs/> .....20M |doi=10.3847/1538-3881/ab1cbd |title=A Catalog of Known Galactic K-M Stars of Class I Candidate Red Supergiants in Gaia DR2 |year=2019 |last1=Messineo ...

...find variable stars in NGC 6496. In one of the studies, thirteen variable stars were detected by Dr. Moe Abbas and Dr. Andrew Layden from [[Bowling Green S ...a selection of [[Long-period variable star|long-period variables]] and [[Variable star#Eclipsing binaries|short-period eclipsing binaries]].<ref>{{cite web|t ...

...[[ionised]] [[helium]] found, usually in absorption, in the spectra of hot stars like [[Wolf–Rayet star]]s. The name comes from [[Edward Charles Pickering]] ...er, they are seen in emission in the spectra of Wolf-Rayet stars, as these stars have little or no hydrogen. ...