R Puppis
{{short description|Variable star in the constellation Puppis}}{{confuse|Rho Puppis}}
{{Starbox begin}}
{{Starbox image
|image=
{{Location mark
|image=Puppis constellation map.svg|alt=|float=center|width=240
|label=|position=right
|mark=Red circle.svg|mark_width=10|mark_link=R Puppis
|x=468|y=688
}}
|caption=Location of R Puppis (circled)
}}
{{Starbox observe
| epoch = J2000
| constell = Puppis
}}
{{Starbox character
| variable = SRd
}}
{{Starbox astrometry
| parallax = 0.2440
| p_error = 0.0180
}}
{{Starbox detail
| temperature = {{val|5495|fmt=commas}}; {{nowrap|({{val|4100|68|fmt=commas}}{{snd}}6,500)}}
| luminosity = {{val|96600|26100|fmt=commas}}
| rotational_velocity =
}}
{{Starbox catalog
| names = CD−31°4910, GSC 07106-03582, HIP 37415, HR 2974, HD 62058
}}
{{Starbox reference
| Simbad = R+Puppis
}}
{{Starbox end}}
File:NGC 2439 DSS.jpg, with R Puppis the brightest star]]
R Puppis is a variable star in the constellation Puppis. It is a rare yellow hypergiant and a candidate member of the open cluster NGC 2439. It is also an MK spectral standard for the class G2 0-Ia.
Variability
File:RPupLightCurve.png light curve for R Puppis, plotted from ASAS data]]
R Puppis was identified as a variable star in 1879, and described as having a range of over a magnitude. Numerous observations over the following 100 years failed to confirm the variations, until the 1970s when clear brightness changes were observed. These were confirmed by later observations, but with a total visual amplitude of only about 0.2 magnitudes.
Variable stars such as R Puppis have been described as pseudo-Cepheids, because they lie above the high-luminosity portion of the instability strip and their variations are similar to those of Cepheids although less regular. R Puppis is formally classified as a semiregular variable of type SRd, meaning F, G, or K giants or supergiants.
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References
{{reflist|refs=
{{cite Gaia DR2|5598101850119654272}}
{{cite Gaia DR3|5598101850119654272}}
| bibcode=2022yCat.1354....0A
| title=VizieR Online Data Catalog: StarHorse2, Gaia EDR3 photo-astrometric distances (Anders+, 2022)
| last1=Anders |first1=F. |last2=Khalatyan |first2=A.
| last3=Queiroz |first3=A. B. A. |last4=Chiappini |first4=C.
| last5=Ardevol |first5=J. |last6=Casamiquela |first6=L.
| last7=Figueras |first7=F. |last8=Jimenez-Arranz |first8=O.
| last9=Jordi |first9=C. |last10=Monguio |first10=M.
| last11=Romero-Gomez |first11=M. |last12=Altamirano |first12=D.
| last13=Antoja |first13=T. |last14=Assaad |first14=R.
| last15=Cantat-Gaudin |first15=T. |last16=Castro-Ginard |first16=A.
| last17=Enke |first17=H. |last18=Girardi |first18=L.
| last19=Guiglion |first19=G. |last20=Khan |first20=S.
| last21=Luri |first21=X. |last22=Miglio |first22=A.
| last23=Minchev |first23=I. |last24=Ramos |first24=P.
| last25=Santiago |first25=B. X. |last26=Steinmetz |first26=M.
| journal=Vizier Online Data Catalog |year=2022 }}
{{cite journal |bibcode=1978IBVS.1473....1S |title=R Pup - a Variable after all |journal=Information Bulletin on Variable Stars |date=September 1978 |last1=Stift |first1=M. J. |volume=1473 |page=1 }}
{{cite journal |bibcode=1983AJ.....88..386E |doi=10.1086/113323 |title=Pseudocepheids. I. R Puppis, HR 4441, HR 4511, and AI CMi |author1=Eggen, O. J. |journal=Astronomical Journal |volume=88 |pages=386–403 |date=March 1983 }}
| last1=Keenan | first1=Philip C. | last2=McNeil | first2=Raymond C.
| title=The Perkins catalog of revised MK types for the cooler stars
| journal=Astrophysical Journal Supplement Series
| volume=71 | pages=245 | year=1989
| bibcode=1989ApJS...71..245K | doi=10.1086/191373 | s2cid=123149047 }}
| last1=Garcia | first1=B.
| title=A list of MK standard stars
| journal=Bulletin d'Information du Centre de Données Stellaires
| volume=36 | pages=27 | year=1989
| bibcode=1989BICDS..36...27G }}
}}
{{Stars of Puppis}}
{{DEFAULTSORT:R Puppis}}