Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Antlia |
Right ascension | 09h 56m 54.09215s[2] |
Declination | −27° 28′ 30.5575″[2] |
Apparent magnitude (V) | 6.32 (+0.01)[3] |
Characteristics | |
Spectral type | A4 V[3] |
B−V color index | 0.173±0.008[4] |
Variable type | δ Sct[3] |
Astrometry | |
Radial velocity (Rv) | +18.2±0.8[5] km/s |
Proper motion (μ) | RA: −72.627[2] mas/yr Dec.: +23.234[2] mas/yr |
Parallax (π) | 6.8977 ± 0.0578 mas[2] |
Distance | 473 ± 4 ly (145 ± 1 pc) |
Absolute magnitude (MV) | 0.33[4] |
Details[6] | |
Mass | 2.41±0.05 M☉ |
Luminosity | 66.8+11.7 −10.0 L☉ |
Temperature | 7,745+53 −71 K |
Rotational velocity (v sin i) | 218.9±1.7[7] km/s |
Other designations | |
Database references | |
SIMBAD | data |
BF Antliae, or HD 86301, is a variable star in the southern constellation of Antlia. It has a baseline apparent visual magnitude of 6.32,[3] which indicates it lies near the lower limit of visibility for faint stars. The distance to BF Ant, as determined from its annual parallax shift of 6.9 mas,[2] is 473 light years. It is moving further away with a heliocentric radial velocity of +18 km/s.[5]
This is an A-type main-sequence star with a stellar classification of A4 V[3] that is at the end of its main sequence lifespan.[6] It is a Delta Scuti variable that varies by 0.01 of a magnitude.[3] These are short-period (six hours at most) pulsating stars that have been used as standard candles and as subjects to study astroseismology.[9] Handler and Shobbrook (2002) noted that the star lies near the "hot luminous border of the δ Scuti instability strip", and it appears "multiperiodic with a time scale of 3.8–6 hours".[10]
BF Antliae is spinning rapidly with a projected rotational velocity of 219 km/s.[7] It has 2.41 times the mass of the Sun and is radiating 67 times the Sun's luminosity from its photosphere at an effective temperature of 7,745 K.[6]
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