Highly luminous binary star system in the constellation Carina
HD 93250
Observation dataEpoch J2000 Equinox J2000
Constellation
Carina
Right ascension
10h 44m 45.028s [ 1]
Declination
−59° 33′ 54.68″[ 1]
Apparent magnitude (V)
7.41[ 2]
Characteristics
Spectral type
O4 IV(fc)[ 3]
U−B color index
−0.85[ 2]
B−V color index
+0.17[ 2]
Astrometry Radial velocity (Rv )11.6[ 4] km/s Proper motion (μ) RA: −7.116[ 1] mas /yr Dec.: +3.081[ 1] mas /yr Parallax (π)0.4115 ± 0.0199 mas [ 1] Distance 7,900 ± 400 ly (2,400 ± 100 pc ) Absolute magnitude (MV )−6.14[ 5]
Orbit [ 6] Period (P) 194.31± 0.39 d Semi-major axis (a) 1.224± 0.028 mas Eccentricity (e) 0.217± 0.011Inclination (i) 22± 41 °Longitude of the node (Ω) 59± 20 °Argument of periastron (ω) (secondary) 171± 24 °
Details[ 5] Radius 15.9 R ☉ Luminosity 1,000,000 L ☉ Surface gravity (log g )3.96 cgs Temperature 46,000 K Rotational velocity (v sin i )130 km/s Age 1.3 Myr
A Mass 49[ 6] M ☉
Other designations 1E 104248-5918.0,
XMMU J104444.8-593354,
ALS 1859,
2E 2317,
HIP 52558,
CD -58°3537,
GC 14791,
CGO 246,
GCRV 25947,
PPM 339400,
Trumpler 16 180,
SAO 238423,
Trumpler 14 101,
TYC 8626-2075-1,
CPC 20°3140,
GOS G287.51-00.54 01,
CPD −58°2661,
GSC 08626-02075
Database references SIMBAD data
HD 93250 is a highly luminous hot blue binary star in the Carina Nebula in the constellation Carina .
^ a b c d e Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties" . Astronomy and Astrophysics . 674 : A1. arXiv :2208.00211 . Bibcode :2023A&A...674A...1G . doi :10.1051/0004-6361/202243940 . S2CID 244398875 .
Gaia DR3 record for this source at VizieR .
^ a b c Antokhin, I. I.; Rauw, G.; Vreux, J.-M.; Van Der Hucht, K. A.; Brown, J. C. (2008). "XMM-Newton X-ray study of early type stars in the Carina OB1 association". Astronomy and Astrophysics . 477 (2): 593. arXiv :0711.3612 . Bibcode :2008A&A...477..593A . doi :10.1051/0004-6361:20065711 . S2CID 82888037 .
^ Maíz Apellániz, J.; Sota, A.; Arias, J. I.; Barbá, R. H.; Walborn, N. R.; Simón-Díaz, S.; Negueruela, I.; Marco, A.; Leão, J. R. S.; Herrero, A.; Gamen, R. C.; Alfaro, E. J. (2016). "The Galactic O-Star Spectroscopic Survey (GOSSS). III. 142 Additional O-type Systems" . The Astrophysical Journal Supplement Series . 224 (1): 4. arXiv :1602.01336 . Bibcode :2016ApJS..224....4M . doi :10.3847/0067-0049/224/1/4 . S2CID 55658165 .
^ Rauw, G.; Nazé, Y.; Fernández Lajús, E.; Lanotte, A. A.; Solivella, G. R.; Sana, H.; Gosset, E. (2009). "Optical spectroscopy of X-Mega targets in the Carina nebula - VII. On the multiplicity of Tr16-112, HD93343 and HD93250" . Monthly Notices of the Royal Astronomical Society . 398 (3): 1582–1592. arXiv :0906.2681 . Bibcode :2009MNRAS.398.1582R . doi :10.1111/j.1365-2966.2009.15226.x . S2CID 13890955 .
^ a b Repolust, T.; Puls, J.; Herrero, A. (2004). "Stellar and wind parameters of Galactic O-stars. The influence of line-blocking/blanketing" . Astronomy and Astrophysics . 415 : 349. Bibcode :2004A&A...415..349R . doi :10.1051/0004-6361:20034594 .
^ a b Le Bouquin, J. -B; Sana, H.; Gosset, E.; De Becker, M.; Duvert, G.; Absil, O.; Anthonioz, F.; Berger, J. -P.; Ertel, S.; Grellmann, R.; Guieu, S.; Kervella, P.; Rabus, M.; Willson, M. (2017). "Resolved astrometric orbits of ten O-type binaries". Astronomy and Astrophysics . 601 : A34. arXiv :1608.03525 . Bibcode :2017A&A...601A..34L . doi :10.1051/0004-6361/201629260 . S2CID 53686222 .