HD 63032

{{Short description|Binary star system in the constellation Puppis}}

{{Starbox begin

| name=c Puppis }}

{{Starbox image

| image = 250px

| caption = The field of cluster NGC 2451; c Puppis is the brightest star in the frame

}}

{{Starbox observe

| epoch=J2000

| ra={{RA|07|45|15.29613}}

| dec={{DEC|-37|58|06.9069}}

| constell=Puppis

| appmag_v=3.61

}}

{{Starbox character

| class=K2.5Ib-IIa（K5IIa） + B9V

| u-b=1.72

| b-v=1.73

| appmag_2_passband=U

| appmag_2=7.06

| appmag_3_passband=B

| appmag_3=5.34

| appmag_4_passband=R

| appmag_4=2.26

| appmag_5_passband=I

| appmag_5=1.26

| appmag_6_passband=J

| appmag_6=0.68

| appmag_7_passband=H

| appmag_7=-0.075 ± 0.220

| appmag_8_passband=K

| appmag_8=-0.47

| variable=

}}

{{Starbox astrometry

| radial_v=16.83 ± 0.14

| prop_mo_ra={{val|-10.54}}

| prop_mo_dec={{val|5.584}}

| pm_footnote=

| parallax = 2.9460

| p_error = 0.1482

| parallax_footnote ={{cite Gaia DR3|5538814190283894656}}

| dist_pc = {{val|341.7|20.5|19.5}}

| dist_ly = {{val|{{convert|341.7|pc|ly|disp=number|sigfig=4}}|{{convert|20.5|pc|ly|disp=number|sigfig=3}}|{{convert|10.5|pc|ly|disp=number|sigfig=3}}|fmt=commas}}

| dist_footnote =

}}

{{Starbox detail

| component1=A

| mass={{val|12.1|1.2}}

| radius={{val|274|14}}{{snd}}301

| luminosity=15,152

| temperature=3,781

| age_myr = {{val|15.8|0.4}}

| component2=B

| radius2={{val|2.0|0.3}}

| temperature2=10,200 ± 300

}}

{{Starbox catalog

| names= CD−37 3863, CPD−37 1558, HD 63032, HIP 37819, HR 3017, SAO 198398

}}

{{Starbox reference

| Simbad=HIP+37819

}}

c Puppis, also known as HD 63032 and HR 3017, is a spectroscopic binary star in the constellation Puppis. Its apparent magnitude is of 3.61, making it the eight-brightest star in Puppis. The system is the brightest member of the open cluster NGC 2451, over two magnitudes brighter than every other star in the cluster. As the turnoff point of the cluster is currently around B7, the parameters of the system fit with cluster membership.

The primary component of the system is a red supergiant or bright giant of spectral classification K2.5Ib-IIa. It is twelve times more massive than the Sun, and is estimated 16 million years old. At this evolutionary stage, it has expanded to 280 times the size of the Sun and is 15,000 more luminous. Its surface has cooled to an effective temperature of 3,781 K, giving it a red-orange hue. The secondary component is a late B-type star, about two times the size of the Sun. c Puppis was first discovered to be a spectroscopic binary in 1982, by D. Groote and D. Reimers.

References

{{reflist|refs=

{{Citation |last1=McDonald |first1=I. |last2=Zijlstra |first2=A. A. |last3=Boyer |first3=M. L. |date=2012-11-01 |title=Fundamental parameters and infrared excesses of Hipparcos stars |bibcode=2012MNRAS.427..343M |journal=Monthly Notices of the Royal Astronomical Society |volume=427 |pages=343–357 |doi=10.1111/j.1365-2966.2012.21873.x |doi-access=free |issn=0035-8711|arxiv=1208.2037 }} [https://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/MNRAS/427/343&HIP=37819 c Puppis' database entry] at VizieR.

{{cite journal |last1=Groote |first1=D. |last2=Reimers |first2=D. |title=Detection of a late B star companion of the bright cluster giant c Pup = HD 63032 |journal=Astronomy and Astrophysics |volume=119 |issue=2 |pages=319–320 |date=1983 |bibcode=1983A&A...119..319G}}

{{Cite journal |last1=Kervella |first1=Pierre |last2=Arenou |first2=Frédéric |last3=Thévenin |first3=Frédéric |date=2022-01-01 |title=Stellar and substellar companions from Gaia EDR3. Proper-motion anomaly and resolved common proper-motion pairs |bibcode=2022A&A...657A...7K |journal=Astronomy and Astrophysics |volume=657 |pages=A7 |doi=10.1051/0004-6361/202142146 |issn=0004-6361|arxiv=2109.10912 }} [https://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A%2BA/657/A7&HIP=37819 c Puppis' database entry] at VizieR.

{{cite journal|bibcode=2002yCat.2237....0D|title=VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system|journal=CDS/ADC Collection of Electronic Catalogues|volume=2237|pages=0|last1=Ducati|first1=J. R.|year=2002}}

{{cite journal

| last1=Eggleton | first1=P. P.

| last2=Tokovinin | first2=A. A.

| title=A catalogue of multiplicity among bright stellar systems

| journal=Monthly Notices of the Royal Astronomical Society

| volume=389 | issue=2 | pages=869–879 | date=September 2008

| doi=10.1111/j.1365-2966.2008.13596.x

| doi-access=free

| bibcode=2008MNRAS.389..869E

| arxiv=0806.2878

| s2cid=14878976

}}

{{Cite journal |last1=Bailer-Jones |first1=C. A. L. |last2=Rybizki |first2=J. |last3=Fouesneau |first3=M. |last4=Demleitner |first4=M. |last5=Andrae |first5=R. |date=2021-03-01 |title=Estimating distances from parallaxes. V: Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3 |journal=The Astronomical Journal |volume=161 |issue=3 |pages=147 |doi=10.3847/1538-3881/abd806 |doi-access=free |arxiv=2012.05220 |bibcode=2021AJ....161..147B |issn=0004-6256}} Data about this star can be seen [https://dc.zah.uni-heidelberg.de/gedr3dist/q/cone/form here].

{{cite journal |bibcode=2003yCat.2246....0C |title=VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) |journal=CDS/ADC Collection of Electronic Catalogues |pages=II/246 |volume=2246 |last1=Cutri |first1=Roc M. |last2=Skrutskie |first2=Michael F. |last3=Van Dyk |first3=Schuyler D. |last4=Beichman |first4=Charles A. |last5=Carpenter |first5=John M. |last6=Chester |first6=Thomas |last7=Cambresy |first7=Laurent |last8=Evans |first8=Tracey E. |last9=Fowler |first9=John W. |last10=Gizis |first10=John E. |last11=Howard |first11=Elizabeth V. |last12=Huchra |first12=John P. |last13=Jarrett |first13=Thomas H. |last14=Kopan |first14=Eugene L. |last15=Kirkpatrick |first15=J. Davy |last16=Light |first16=Robert M. |last17=Marsh |first17=Kenneth A. |last18=McCallon |first18=Howard L. |last19=Schneider |first19=Stephen E. |last20=Stiening |first20=Rae |last21=Sykes |first21=Matthew J. |last22=Weinberg |first22=Martin D. |last23=Wheaton |first23=William A. |last24=Wheelock |first24=Sherry L. |last25=Zacarias |first25=N. |year=2003 |url=http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=II/246 }}

{{citation | last1=Mermilliod | first1=J. C. | last2=Mayor | first2=M. | last3=Udry | first3=S. | title=Red giants in open clusters. XIV. Mean radial velocities for 1309 stars and 166 open clusters | journal=Astronomy and Astrophysics | volume=485 | issue=1 | pages=303–314 |date= 2008 | doi=10.1051/0004-6361:200809664 | url=https://www.aanda.org/articles/aa/pdf/2008/25/aa09664-08.pdf | bibcode=2008A&A...485..303M | doi-access=free }}

{{cite web |title=The Colour of Stars |url=https://www.atnf.csiro.au/outreach/education/senior/astrophysics/photometry_colour.html |website=Australia National Telescope Facility |date=6 March 2024 |access-date=2024-05-27 }}

{{Cite journal |last1=Tetzlaff |first1=N. |last2=Neuhäuser |first2=R. |last3=Hohle |first3=M. M. |date=2011-01-01 |title=A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun |journal=Monthly Notices of the Royal Astronomical Society |volume=410 |issue=1 |pages=190–200 |doi=10.1111/j.1365-2966.2010.17434.x |doi-access=free |arxiv=1007.4883 |bibcode=2011MNRAS.410..190T |issn=0035-8711}} [https://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/MNRAS/410/190&recno=2636 c Puppis' database entry] at VizieR.

}}

Category:Puppis

Category:K-type supergiants

Category:K-type giants

Category:Spectroscopic binaries

Category:Durchmusterung objects