HD 56405
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Canis Major |
Right ascension | 07h 16m 14.5528s[1] |
Declination | −15° 35′ 08.485″[1] |
Apparent magnitude (V) | 5.4[2] |
Characteristics | |
Spectral type | A1V |
B−V color index | 0.07[2] |
Astrometry | |
Radial velocity (Rv) | 10 ± 5 km/s |
Proper motion (μ) | RA: -45.2[3] mas/yr Dec.: -15.2[3] mas/yr |
Parallax (π) | 11.79 ± 0.85 mas |
Distance | 237.1[2] ly (72.7[2] pc) |
Details | |
Mass | 12.12[1] M☉ |
Other designations | |
HIP 35180, HR 2758, TYC 5965-363-1[2] | |
Database references | |
SIMBAD | data |
HD 56405 (also known as HIP 35180) is a main sequence star in the Canis Major constellation. On the eastern side of HD 56405 is the open cluster NGC 2360 also known as Caroline's Cluster.[4] It was classed as a Lambda Boötis star,[5] but more recently this classification has been rejected by astronomers due to the star having an inconsistent UV flux and RV variability and being a high vsin i A2 Va standard star.[6]
References
- 1 2 3 "HD 56405 -- Star". SIMBAD. Retrieved 13 November 2017.
- 1 2 3 4 5 "The star HR 2758". In the sky. Retrieved 13 November 2017.
- 1 2 "HD 56405". Sky Map. Retrieved 19 November 2017.
- ↑ Streicher, Magda (December 2005). "Deepsky Delights" (PDF). The Astronomical Society of Southern Africa. p. 234–36. Retrieved 13 November 2017.
- ↑ "MK classification for visual binary components". Researchgate. March 1976. Retrieved 19 November 2017.
- ↑ "An Evaluation of the Membership Probability of 212 λ Boo Stars. I. A Catalogue" (PDF). Astronomical Society of Australia. July 6, 2015. Retrieved 19 November 2017.
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