HD 23005
  | |
| Observation data ICRS )
| |
|---|---|
| Constellation | Camelopardalis |
| Right ascension | 03h 46m 00.94002s[1] |
| Declination | +67° 12′ 05.7682″[1] |
| Apparent magnitude (V) | 5.78±0.01[2] |
| Characteristics | |
| Spectral type | F1 IVnn[3] |
| U−B color index | +0.05[4] |
| B−V color index | +0.34[4] |
| Variable type | candidate γ Doradus[3] |
| Absolute magnitude (MV) | +2.07[6] |
| Details | |
Gyr | |
| Database references | |
| SIMBAD | data |
HD 23005, also known as HR 1124, is a solitary,Gaia DR3 parallax measurements but is receding with a heliocentric radial velocity of 4.9 km/s.[5] At its current distance, HD 23005's brightness is diminished by 0.15 magnitudes due to extinction from interstellar dust.[16] It has an absolute magnitude of +2.07.[6]
The star has been given several
F-type star
.
HD 23005's newest spectral class is F1 IVnn, which indicates that it is an
projected rotational velocity of 66 km/s. [12] A 2016 variable star survey identified HD 23005 as a candidate γ Doradus variable.[3]
References
- ^ S2CID 244398875. Gaia DR3 record for this source at VizieR.
- ISSN 0004-6361.
- ^ ISSN 0035-8711.
- ^ a b Imagawa, Fumihiko (February 1967). "Observational Results of Three-color Photometry for F-type Stars (II)". Memoirs of the College of Science, University of Kyoto. Series A. 31 (2): 93–100.
- ^ S2CID 119231169.
- ^ S2CID 119257644.
- ^ ISSN 0004-6361.
- ^ ISSN 0004-6361.
- S2CID 166227927.
- ^ ISSN 0004-6361.
- ^ ISSN 0035-8711.
- ^ S2CID 54046583.
- ^ ISSN 0004-6361.
- ^ "HD 23005". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved January 20, 2023.
- S2CID 14878976.
- ISSN 0035-8711.
- ISSN 0004-6280.
- ISSN 0004-637X.
- ISSN 0004-6280.
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