HD 110432
Location of BZ Crucis (circled). The other star shown overlapping/underlying the dark nebula is HD 109000 (HR 4771) which is a red/brown star about half the distance to the nebula, having parallax of 12.8 ± 0.05 thus about 250 light years away[1] | |
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Crux |
Right ascension | 12h 42m 50.2656s[1] |
Declination | −63° 03′ 31.048″[1] |
Apparent magnitude (V) | 5.24 - 5.45[2] |
Characteristics | |
Spectral type | B1IVe[3] |
U−B color index | −0.82[4] |
B−V color index | +0.27[4] |
Variable type | γ Cas[2] |
Absolute magnitude (MV) | −2.56[6] |
Details | |
Rotational velocity (v sin i) | 300–400[3] km/s |
HIP 62027.[8] | |
Database references | |
SIMBAD | data |
HD 110432 is a Be star in the south-east of Crux, behind the center of the southern hemisphere's dark
variable star designation BZ Crucis. It is not known to be a member of a binary system, although it is probably a member of the open cluster NGC 4609. This star is moderately luminous in the X-ray band, with a variable energy emission of 1032–33 erg s−1 in the range 0.2−12 keV. The X-ray emission may be caused by magnetic activity, or possibly by accretion onto a white dwarf companion.[3]
Distance
The distance of 388 Gaia Data Release 2 is even further at 420 pc.[1]
References
- ^ .
- ^ Bibcode:2009yCat....102025S.
- ^ S2CID 14593244.
- ^ Bibcode:1973MNSSA..32...11C.
- Bibcode:1967IAUS...30...57E.
- S2CID 119257644.
- S2CID 11256230.
- Centre de Données astronomiques de Strasbourg. Retrieved 2010-12-09.
- S2CID 250669202. Retrieved 17 December 2021.
- S2CID 18759600.