G 99-47
Coordinates: 05h 56m 25.47s, +05° 21′ 48.6″
Observation data J2000[2]
| |
---|---|
Constellation | Orion |
Right ascension | 05h 56m 25.47s[2] |
Declination | +05° 21′ 48.6″[2] |
Apparent magnitude (V) | 14.105[3] |
Characteristics | |
Spectral type | DAP8.9[4] |
Apparent magnitude (B) | 14.69[2] |
Apparent magnitude (V) | 14.10[2] |
Apparent magnitude (R) | 14.0[2] |
Apparent magnitude (I) | 13.6[2] |
Apparent magnitude (J) | 12.930 ± 0.022[2] |
Apparent magnitude (H) | 12.720 ± 0.025[2] |
Apparent magnitude (K) | 12.653 ± 0.024[2] |
Absolute magnitude (MV) | 14.59[3][6][note 1] |
Details | |
Gyr | |
Database references | |
SIMBAD | data |
G 99-47 (V1201 Orionis) is a nearby degenerate star (
Gliese 915
.
The mass of G 99-47 is 0.71±0.03
Gyr.[4] Due almost equal to the Sun's temperature, GJ 1087 should appear almost the same white color as the Sun. The white dwarf has a strong magnetic field, with measured vertical component near surface equal to 560 T.[7]
See also
Notes
References
- S2CID 56285149.
- ^ Centre de Données astronomiques de Strasbourg. Retrieved 2011-11-01.
- ^ a b c d e f g h i j k l
Holberg, J. B.; Sion; Oswalt; McCook; Foran; Subasavage (2008). "A New Look at the Local White Dwarf Population". S2CID 122855486.
- ^ a b c d e
Sion, Edward M.; Holberg; Oswalt; McCook; Wasatonic (2009). "The White Dwarfs within 20 Parsecs of the Sun: Kinematics and Statistics". S2CID 119284418.
- ^ .
- ^ a b Yale Trigonometric Parallaxes, Fourth Edition (van Altena+ 1995)
- S2CID 222290583