145 G. Canis Majoris
Appearance
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Canis Major |
Right ascension | 07h 16m 36.83456s[1] |
Declination | −23° 18′ 56.1383″[1] |
Apparent magnitude (V) | 4.79[2] |
Characteristics | |
Spectral type | K3Ib-[3] or K4III[4] |
B−V color index | 1.710[2] |
Details | |
If a giant star | |
Myr | |
Database references | |
SIMBAD | data |
145 G. Canis Majoris (HD 56577) is a singlesupergiant star in the southern constellation of Canis Major. This star is Gould's 145th of Canis Major in his Uranometria Argentina. [11] Kostjuk erroneously lists it as simply "145 CMa". SIMBAD follows this error in its object query result as "* 145 CMa – Star".[12]
The properties and evolutionary state of 145 G. CMa are disputed, it being classed either as a young massive supergiant or a somewhat older and less massive giant. It has been given two MK
(corresponding to a giant). Tezzlaff et al. gives a large mass of 7.8K-type stars.[13]
Based on the assumption that it is a
Gaia DR2 parallax, it would have a luminosity of 14,000 L☉, rather high for a giant.[5] An older measurement based on the Hipparcos distance of 435 parsecs (1,420 ly) give a lower luminosity of 5,960 L☉.[14]
The star is one component of a close
″.[15] The two stars appear to be unrelated and the close alignment accidental, with HD 56578 being a much closer and less luminous Am star.[16]
Notes
- ^ a b Applying the Stefan–Boltzmann law with a nominal solar effective temperature of 5,772 K:
- .
References
- ^ S2CID 244398875. Gaia DR3 record for this source at VizieR.
- ^ S2CID 118505114.
- ^ doi:10.1086/191373.
- ^ Bibcode:1988mcts.book.....H.
- ^ .
- ^ S2CID 118629873.
- ^ ISSN 0035-8711.
- .
- ^ "HD 56577". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-01-06.
- S2CID 14878976.
- ^ Gould, B. A., (2009) Uranometria Argentina, (Reprinted and updated by Pilcher, F.)[1] Archived 2016-03-05 at the Wayback Machine
- ^ SIMBAD query * 145 CMa – Star
- ^ "The Colour of Stars". Australia National Telescope Facility. Retrieved 2024-05-27.
- .
- doi:10.1086/323920.
- .