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Star in the constellation Auriga From Wikipedia, the free encyclopedia
HD 37519 or Andrew's Star is a star in the northern constellation Auriga. It has a blue-white hue and is dimly visible to the naked eye with an apparent visual magnitude of 6.04.[2] The distance to HD 37519 is approximately 810 light years based on parallax, but it is drifting closer with a radial velocity of −10 km/s.[5]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Auriga |
Right ascension | 05h 40m 35.90737s[1] |
Declination | +31° 21′ 29.5262″[1] |
Apparent magnitude (V) | 6.04[2] |
Characteristics | |
Spectral type | B9.5III-IV(p)? (Hg?)[3] |
U−B color index | −0.21[2] |
B−V color index | +0.05[2] |
Variable type | suspected[4] |
Astrometry | |
Radial velocity (Rv) | −10.2±3.4[5] km/s |
Proper motion (μ) | RA: −5.051[1] mas/yr Dec.: −8.187[1] mas/yr |
Parallax (π) | 4.0335 ± 0.1112 mas[1] |
Distance | 810 ± 20 ly (248 ± 7 pc) |
Absolute magnitude (MV) | −0.43[6] |
Details | |
Radius | 3.0[7] R☉ |
Luminosity | 110[8] L☉ |
Temperature | 8,289[8] K |
Rotational velocity (v sin i) | 195[9] km/s |
Age | 375[6] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Cowley in 1972 found a stellar classification of B9.5III-IV(p)? (Hg?) for this star,[3] suggesting it is an evolved B-type star and a suspected chemically peculiar star of the mercury-manganese type.[11] It is estimated to be 375 million years old and with a high rate of spin, showing a projected rotational velocity of 195 km/s.[9] In March 1964, a suspected flare of HD 37519 was detected that increased the star's brightness by about three magnitudes. Smaller variations of up to two magnitudes were detected a few days later,[12] suggesting there might be a flare star companion. However, follow-up observations failed to confirm the variability.[13] The star is radiating 110[8] times the luminosity of the Sun from its photosphere at an effective temperature of 8,289 km/s.[8]
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