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| Description of NGC 7099 |
Messier 30 (also known as M30 or NGC 7099) is a globular cluster in the Capricornus constellation. It was discovered by Charles Messier in 1764. M30 is at a distance of about 26,000 light-years away from Earth.
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Image of the cluster from the Digital Sky Survey |
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(0 comments in the database at the moment) | Selected biblio  | | Paper n. 1 |
Mucciarelli, A.; Lovisi, L.; Lanzoni, B.; Ferraro, F. R.
The Helium Abundance in the Metal-poor Globular Clusters M30 and NGC 6397
2014, The Astrophysical Journal, Volume 786, Issue 1, article id. 14, 8 pp.
(NGC 7099 NGC 6397 ) | | Paper n. 2 |
Davidge, T. J.
Near-Infrared Photometry of the Core-Collapsed Metal-Poor Globular Cluster NGC 5946 and NGC 7099
1995, Astronomical Journal v.110, p.1177
(NGC 5946 NGC 7099 ) | | Paper n. 3 |
Buonanno, R.; Caloi, V.; Castellani, V.; Corsi, C. E.; Ferraro, I.;
Piccolo, F.
CCD photometry of stars in the metal-poor globular cluster NGC 7099 (M30)
1988, Astronomy and Astrophysics Supplement Series, vol. 74, no. 3, Sept. 1998
(NGC 7099 cmd ) | | See all items
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