NGC 2360
J2000 epoch) | |
---|---|
Right ascension | 07h 17m 43s[1] |
Declination | −15° 38′ 29″[1] |
Apparent magnitude (V) | 7.2[2] |
Apparent dimensions (V) | 13′[2] |
Physical characteristics | |
Other designations | Caroline's Cluster,[3] Caldwell 58, Cr 134, Mel 64[3] |
Associations | |
Constellation | Canis Major |
NGC 2360 (also known as Caroline's Cluster
American astronomer Olin J. Eggen surveyed the cluster in 1968, concluding that the brightest star in the field, magnitude-8.96 HD 56847, is likely to lie in the field and not a true member of the cluster. He also identified one or possibly two blue stragglers.[7] These are unexpectedly hot and luminous stars that appear younger than surrounding stars, and have likely developed by sucking matter off companion stars.[8] Four are now recognised to be in the cluster.[9] By analysing the masses of the smallest stars that have evolved into red giants—namely, stars of 1.8 or 1.9 solar masses—Swiss astronomers Jean-Claude Mermilliod and Michel Mayor were able to date the age of the cluster at 2.2 billion years.[10] The cluster has a diameter of around 15 light-years and is located 3700 light-years from Earth.[5]
Sirius and M41 (lower right), M50 (upper left), and NGC 2360 (lower left) |
Notes
- ^ a b "Results for NGC 2360". NGC/IC Project Database. Archived from the original on 2012-05-20. Retrieved 2010-12-03.
- ^ a b c "SEDS Online NGC Database". Results for NGC 2360. Retrieved 2010-12-03.
- ^ a b c "NGC 2360". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2010-12-03.
- ^ S2CID 118428465.
- ^ ISBN 978-0-521-82796-6.
- ^ Streicher, Magda (April 2006). "Caroline Herschel's Deepsky Discoveries" (PDF). Deepsky Delights. The Astronomical Society of Southern Africa. pp. 234–36. Retrieved 16 March 2014.
- doi:10.1086/149526.
- ^ Fellman, Megan (17 October 2011). "Astronomers Explain 'Blue Stragglers'". News. Evanston, Illinois: Northwestern University. Retrieved 18 March 2014.
- .
- Bibcode:1990A&A...237...61M.
External links
- NGC 2360 on