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HD 69863

From Wikipedia, the free encyclopedia
Binary star system in the constellation Carina
This article is about C Carinae. Forc Carinae, seeHD 76728.
HD 69863
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationCarina
A
Right ascension08h 15m 16.42864s[1]
Declination−62° 54′ 56.5007″[1]
Apparent magnitude (V)5.27[2]
B
Right ascension08h 15m 16.47622s[3]
Declination−62° 54′ 54.8700″[3]
Apparent magnitude (V)7.62[2]
Characteristics
Spectral typeA2V[4] + F2V[5]
B−Vcolor index0.086±0.003[6]
Astrometry
Radial velocity (Rv)4.0±3.7[6] km/s
Absolute magnitude (MV)0.71[6]
A
Proper motion (μ)RA: −26.674[1]mas/yr
Dec.: -12.060[1]mas/yr
Parallax (π)12.5410±0.1714 mas[1]
Distance260 ± 4 ly
(80 ± 1 pc)
B
Proper motion (μ)RA: −20.911[3] mas/yr
Dec.: -14.466[3] mas/yr
Parallax (π)12.7714 ± 0.0329 mas[3]
Distance255.4 ± 0.7 ly
(78.3 ± 0.2 pc)
Details
A
Mass2.10+0.20
−0.17
[7] M
Luminosity42[8] L
Surface gravity (log g)3.90±0.14[7] cgs
Temperature8774+601
−210
[1] K
Rotational velocity (v sin i)191[9] km/s
B
Radius1.43+0.12
−0.08
[3] R
Luminosity3.966±0.016[3] L
Temperature6806+203
−258
[3] K
Age635±88[7] Myr
Other designations
RMK8,C Carinae,CPD−62°985,HD 69863,HIP 40429,HR 3260,CCDM J08153-6255[10]
A:GC 11275,SAO 250164
B:GC 11276,SAO 250165
Database references
SIMBADdata

HD 69863 is abinary star[11] system in the southernconstellation ofCarina. It is visible to the naked eye as a dim point of light with a combinedapparent visual magnitude of 5.16.[6] The system is located at a distance of about255 light years from theSun based onparallax.[1][3] The dual nature of this system was announced in 1832 by German astronomerCarl Rümker.[12] As of 2015, the pair had anangular separation of4.10 along aposition angle of 70°.[2]

The brighter primary, designated component A, has a visual magnitude of 5.27[2] and is anA-type main-sequence star with astellar classification of A2V.[4] It is 635[7] million years old and is spinning with aprojected rotational velocity of 191 km/s.[9] The star has 2.1 times themass of the Sun.[7]

The magnitude 7.62[2] companion, component B, is aF-type main-sequence star with a class of F2V.[5] It is radiating four[3] times theluminosity of the Sun from itsphotosphere at aneffective temperature of 6,806 K.[3] The system is a source forX-ray emission, which is most likely coming from the secondary.[13]

References

[edit]
  1. ^abcdefgBrown, A. G. A.; et al. (Gaia collaboration) (August 2018)."Gaia Data Release 2: Summary of the contents and survey properties".Astronomy & Astrophysics.616. A1.arXiv:1804.09365.Bibcode:2018A&A...616A...1G.doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source atVizieR.
  2. ^abcdeMason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog",The Astronomical Journal,122 (6): 3466,Bibcode:2001AJ....122.3466M,doi:10.1086/323920.
  3. ^abcdefghijkBrown, A. G. A.; et al. (Gaia collaboration) (August 2018)."Gaia Data Release 2: Summary of the contents and survey properties".Astronomy & Astrophysics.616. A1.arXiv:1804.09365.Bibcode:2018A&A...616A...1G.doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source atVizieR.
  4. ^abHouk, Nancy; Cowley, A. P. (1979),Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 1, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan,Bibcode:1978mcts.book.....H
  5. ^abCorbally, C. J. (1984), "Close visual binaries. I. MK classifications",Astrophysical Journal Supplement Series,55: 657,Bibcode:1984ApJS...55..657C,doi:10.1086/190973.
  6. ^abcdAnderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation",Astronomy Letters,38 (5): 331,arXiv:1108.4971,Bibcode:2012AstL...38..331A,doi:10.1134/S1063773712050015,S2CID 119257644.
  7. ^abcdeGullikson, Kevin; et al. (2016), "The Close Companion Mass-ratio Distribution of Intermediate-mass Stars",The Astronomical Journal,152 (2): 40,arXiv:1604.06456,Bibcode:2016AJ....152...40G,doi:10.3847/0004-6256/152/2/40,S2CID 119179065.
  8. ^McDonald, I.; Zijlstra, A. A.; Boyer, M. L. (2012), "Fundamental parameters and infrared excesses of Hipparcos stars",Monthly Notices of the Royal Astronomical Society,427 (1): 343,arXiv:1208.2037,Bibcode:2012MNRAS.427..343M,doi:10.1111/j.1365-2966.2012.21873.x,S2CID 118665352.
  9. ^abRoyer, F.; et al. (October 2002), "Rotational velocities of A-type stars in the northern hemisphere. II. Measurement of v sin i",Astronomy and Astrophysics,393:897–911,arXiv:astro-ph/0205255,Bibcode:2002A&A...393..897R,doi:10.1051/0004-6361:20020943,S2CID 14070763
  10. ^"HD 69863".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2020-01-07. Component B.
  11. ^Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems",Monthly Notices of the Royal Astronomical Society,389 (2):869–879,arXiv:0806.2878,Bibcode:2008MNRAS.389..869E,doi:10.1111/j.1365-2966.2008.13596.x,S2CID 14878976.
  12. ^Letchford, Roderick; et al. (April 2017), "The Southern Double Stars of Carl Rümker I: History, Identification, Accuracy",Journal of Double Star Observations,13 (2):220–232,Bibcode:2017JDSO...13..220L.
  13. ^Schröder, C.; Schmitt, J. H. M. M. (November 2007), "X-ray emission from A-type stars",Astronomy and Astrophysics,475 (2): 677−684,Bibcode:2007A&A...475..677S,doi:10.1051/0004-6361:20077429.
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