NGC 6752(Caldwell 93、Melotte 218)は、くじゃく座の球状星団[2]である。球状星団としては、オメガ星団、きょしちょう座47に次いで全天で3番目に明るい。
出典
- ^ Shapley, Harlow; Sawyer, Helen B. (August 1927), “A Classification of Globular Clusters”, Harvard College Observatory Bulletin (849): 11–14, Bibcode: 1927BHarO.849...11S.
- ^ a b c d “SIMBAD Astronomical Database”. Results for NGC 6752. 2012年5月3日閲覧。
- ^ Boyles, J. et al. (November 2011), “Young Radio Pulsars in Galactic Globular Clusters”, The Astrophysical Journal 742 (1): 51, Bibcode: 2011ApJ...742...51B, doi:10.1088/0004-637X/742/1/51.
- ^ Marks, Michael; Kroupa, Pavel (August 2010), “Initial conditions for globular clusters and assembly of the old globular cluster population of the Milky Way”, Monthly Notices of the Royal Astronomical Society 406 (3): 2000–2012, Bibcode: 2010MNRAS.406.2000M, doi:10.1111/j.1365-2966.2010.16813.x. Mass is from MPD on Table 1.
- ^ a b Forbes, Duncan A.; Bridges, Terry (May 2010), “Accreted versus in situ Milky Way globular clusters”, Monthly Notices of the Royal Astronomical Society 404 (3): 1203–1214, Bibcode: 2010MNRAS.404.1203F, doi:10.1111/j.1365-2966.2010.16373.x.
外部リンク
座標: 19h 10m 52.11s, −59° 59′ 04.4″