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H Centauri








H Centauri


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H Centauri

Observation data
Epoch J2000      Equinox J2000

Constellation

Centaurus

Right ascension
12h 57m 04.35244s[1]

Declination
−51° 11′ 55.5058″[1]

Apparent magnitude (V)
5.163[1]
Characteristics

Spectral type
B7V + B8.5V + B[2]

Apparent magnitude (B)
5.102

Apparent magnitude (V)
5.163

Variable type

ellipsoidal variable[2]
Astrometry
Radial velocity (Rv) 14.55 ± 1.6[2] km/s
Proper motion (μ) RA: −30.15 mas/yr
Dec.: −14.61 mas/yr
Parallax (π) 8.85 ± 0.27 mas
Distance 370 ± 10 ly
(113 ± 3 pc)
Details[2]
Primary
Mass 3.32 ± 0.51 M
Radius 2.09 ± 0.12 R
Luminosity 111 ± 21 L
Surface gravity (log g) 4.3 ± 0.1 cgs
Temperature 13000 K
Secondary
Mass 2.37 ± 0.48 M
Radius 1.67 ± 0.09 R
Luminosity 37 ± 7 L
Surface gravity (log g) 4.4 ± 0.1 cgs
Temperature 10687 ± 52 K
Other designations
H Centauri, V945 Centauri, CD−50 7394, CPD−50 5596, CPC 0 10830, GC 17569, GCRV 7736, GSC 08258-01469, HD 112409, HIC 63210, HIP 63210, HR 4913, PPM 341451, SAO 240407
Database references
SIMBAD data

H Centauri (H Cen), also known as V945 Centauri, is probable triple star system[2] located in the constellation Centaurus. From parallax measurements, it is located 113 parsecs (370 light years) from the sun. It is a member of the Lower Centaurus-Crux (LCC) subgroup of the Scorpius–Centaurus Association.[3]


This system is a double-lined spectroscopic binary formed by two B-type main-sequence star with spectral types B7V and B8.5V. They are in a close (but detached) circular orbit with a period of 0.6496 days and a separation of 5.63 solar radii. Observed at an inclination of 24°, the system is an ellipsoidal variable whose apparent visual magnitude varies from 5.14 to 5.17 over the course of an orbit as the star's visible surface area changes. The system's spectrum contains a third set of spectral lines that are probably from a third star, also of type B.[2]



References[edit]





  1. ^ abc *"* H Cen". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2014-05-14..mw-parser-output cite.citation{font-style:inherit}.mw-parser-output q{quotes:"""""""'""'"}.mw-parser-output code.cs1-code{color:inherit;background:inherit;border:inherit;padding:inherit}.mw-parser-output .cs1-lock-free a{background:url("//upload.wikimedia.org/wikipedia/commons/thumb/6/65/Lock-green.svg/9px-Lock-green.svg.png")no-repeat;background-position:right .1em center}.mw-parser-output .cs1-lock-limited a,.mw-parser-output .cs1-lock-registration a{background:url("//upload.wikimedia.org/wikipedia/commons/thumb/d/d6/Lock-gray-alt-2.svg/9px-Lock-gray-alt-2.svg.png")no-repeat;background-position:right .1em center}.mw-parser-output .cs1-lock-subscription a{background:url("//upload.wikimedia.org/wikipedia/commons/thumb/a/aa/Lock-red-alt-2.svg/9px-Lock-red-alt-2.svg.png")no-repeat;background-position:right .1em center}.mw-parser-output .cs1-subscription,.mw-parser-output .cs1-registration{color:#555}.mw-parser-output .cs1-subscription span,.mw-parser-output .cs1-registration span{border-bottom:1px dotted;cursor:help}.mw-parser-output .cs1-hidden-error{display:none;font-size:100%}.mw-parser-output .cs1-visible-error{font-size:100%}.mw-parser-output .cs1-subscription,.mw-parser-output .cs1-registration,.mw-parser-output .cs1-format{font-size:95%}.mw-parser-output .cs1-kern-left,.mw-parser-output .cs1-kern-wl-left{padding-left:0.2em}.mw-parser-output .cs1-kern-right,.mw-parser-output .cs1-kern-wl-right{padding-right:0.2em}


  2. ^ abcdef Harmanec, P.; Aerts, C.; Prša, A.; Verhoelst, T.; Kolenberg, K. (September 2010). "V945 Centauri = HD 112409: a bright hot short-period binary in a triple system?". Astronomy and Astrophysics. 520: A73, 11 pp. Bibcode:2010A&A...520A..73H. doi:10.1051/0004-6361/201014096.


  3. ^ Chen, Christine H.; Pecaut, Mark; Mamajek, Eric E.; Su, Kate Y. L.; Bitner, Martin (September 2012). "A Spitzer MIPS Study of 2.5-2.0 M ⊙ Stars in Scorpius-Centaurus". The Astrophysical Journal. 756 (2): article 133, 24 pp. arXiv:1207.3415. Bibcode:2012ApJ...756..133C. doi:10.1088/0004-637X/756/2/133.




External links[edit]



  • Alcyone

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