HD 100673

Star in the constellation Centaurus From Wikipedia, the free encyclopedia

HD 100673, also known as A Centauri is a single[11] star in the southern constellation of Centaurus. It is blue-white in hue and is faintly visible to the naked eye with an apparent visual magnitude of +4.62.[1] The star is located at a distance of approximately 430 light-years from the Sun based on stellar parallax.[2] It appears to be drifting further away with a radial velocity of around +6 km/s.[1]

Quick facts Observation data Epoch J2000.0 Equinox J2000.0, Constellation ...
HD 100673
Location of A Centauri (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Centaurus[1]
Right ascension 11h 34m 45.66s[2]
Declination −54° 15 50.7[2]
Apparent magnitude (V) +4.62[1]
Characteristics
Evolutionary stage Main sequence[3]
Spectral type B9V[4]
U−B color index −0.21[5]
B−V color index −0.08[5]
Astrometry
Radial velocity (Rv)+5.7±2.2[1] km/s
Proper motion (μ) RA: −56.17±0.18[2] mas/yr
Dec.: 16.19±0.20[2] mas/yr
Parallax (π)7.65±0.22 mas[2]
Distance430 ± 10 ly
(131 ± 4 pc)
Absolute magnitude (MV)−0.96[1]
Details
Mass3.58±0.05[3] M
Radius4.7[6] R
Luminosity306[3] L
Surface gravity (log g)3.54[6] cgs
Temperature10,600[3] K
Metallicity [Fe/H]0.50[7] dex
Rotation0.733[8] days
Rotational velocity (v sin i)160[3] km/s
Age238[9] Myr
Other designations
A Cen, CPD−53°4637, FK5 2926, GC 15877, HD 100673, HIP 56480, HR 4460, SAO 239189[10]
Database references
SIMBADdata
Close

This is a rapidly rotating Be star, showing an emission-line spectrum on top of the normal absorption spectrum of the star, due to a circumstellar disk of ejected matter. It doesn't show any absorption lines from the disk.[12] It is a B-type main-sequence star with a stellar classification of B9V.[4]

References

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