HD 110073

HD 110073 is a star in the southern constellation Centaurus, near the southern constellation border with Crux. It has the Bayer designation l Centauri (lower case L), while HD 110073 is the star's identifier from the Henry Draper catalogue. This system is faintlyvisible to the naked eye with an apparent visual magnitude of +4.63. It is located at a distance of approximately 365 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +15 km/s.

HD 110073
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Centaurus
Right ascension 12h 39m 52.52839s
Declination −55° 58 31.8904
Apparent magnitude (V) +4.63
Characteristics
Spectral type B8II/III
B−V color index −0.082±0.013
Astrometry
Radial velocity (Rv)+15.1±2.8 km/s
Proper motion (μ) RA: −43.38 mas/yr
Dec.: −25.25 mas/yr
Parallax (π)8.94 ± 0.24 mas
Distance365 ± 10 ly
(112 ± 3 pc)
Absolute magnitude (MV)−0.61
Details
HD 110073 A
Mass4.0±0.2 M
Radius3.7 R
Luminosity385 L
Surface gravity (log g)3.35 cgs
Temperature12,900 K
Metallicity [Fe/H]−0.90 dex
Rotational velocity (v sin i)46±10 km/s
Age129 Myr
HD 110073 B
Mass1.13 M
Luminosity1.2 L
Temperature5,662 K
Other designations
l Cen, CD−39°7748, HD 110073, HIP 61789, HR 4817, SAO 203681
Database references
SIMBADdata

This is a single-lined spectroscopic binary star system that belongs to the Pleiades stream. As of 2011, the pair had a linear projected separation of 130.8±12.1 AU. The primary component is a mercury-manganese star with a stellar classification of B8II/III. These stars are often helium-weak, but this is one of the most normal members of this group in terms of helium abundance. The system is a source for X-ray emission, which is most likely coming from the lower mass companion – it may even be a pre-main-sequence star.

This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.