63 Ophiuchi
Observation data ICRS )
| |
---|---|
Constellation | Sagittarius |
Right ascension | 17h 54m 54.04315s[1] |
Declination | −24° 53′ 13.5444″[1] |
Apparent magnitude (V) | 6.20[2] |
Characteristics | |
Spectral type | O8II((f))[3] |
U−B color index | –0.89[4] |
B−V color index | +0.04[4] |
Absolute magnitude (MV) | −6.0[6] |
Details | |
Rotational velocity (v sin i) | 35[7]-86[8] km/s |
HR 6672, SAO 185928 | |
Database references | |
SIMBAD | data |
63 Ophiuchi is an
Ca II line yields a more modest value of 2,605 ly (799 pc).[10] The star lies only 0.3° north of the galactic plane
.
In 1983, astronomers from the
′ (9–18 pc), surrounded by a diffuse envelope some 65–80′ (14–29 pc) across. At an estimated mass loss rate of (6–8) × 10−6 M☉/yr, it would take the star about (1–5) × 105 years to produce such a nebula from the outflow of its stellar wind.[11]
References
- ^ .
- Bibcode:2002yCat.2237....0D.
- S2CID 118847528.
- ^ doi:10.1086/190852
- Bibcode:1953GCRV..C......0W
- S2CID 55115943.
- ^ S2CID 119258285.
- S2CID 16932907
- S2CID 119268845
- Bibcode:1983SvAL....9..344L