NGC 6101
Appearance
(Redirected from Caldwell 107)
NGC 6101 | |
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![]() Hubble Space Telescope image of the central region of NGC 6101 | |
Observation data (J2000 epoch) | |
Class | X[1] |
Constellation | Apus |
Right ascension | 16h 25m 48.12s[2] |
Declination | –72° 12′ 07.9″[2] |
Apparent magnitude (V) | 9[3] |
Apparent dimensions (V) | 10.7'[3] |
Physical characteristics | |
Metallicity | = –1.76[4] dex |
Estimated age | 12.54 Gyr[4] |
Other designations | Caldwell 107 |
NGC 6101 (also known as Caldwell 107) is a globular cluster in the constellation Apus, which was discovered by James Dunlop and catalogued by him as Δ68. It is located at a distance of about 47,600 light-years from the Sun and about 36,500 light-years from the Galactic Center of the Milky Way. It requires a telescope of at least 20 cm (7.9 in) aperture to resolve individual stars.[3] Research revealed this cluster to contain an unexpected large number of black holes.[5]
References
[edit]- ^ Shapley, Harlow; Sawyer, Helen B. (August 1927), "A Classification of Globular Clusters", Harvard College Observatory Bulletin, 849 (849): 11–14, Bibcode:1927BHarO.849...11S.
- ^ a b Goldsbury, Ryan; et al. (December 2010), "The ACS Survey of Galactic Globular Clusters. X. New Determinations of Centers for 65 Clusters", The Astronomical Journal, 140 (6): 1830–1837, arXiv:1008.2755, Bibcode:2010AJ....140.1830G, doi:10.1088/0004-6256/140/6/1830, S2CID 119183070.
- ^ a b c Dunlop, Storm (2005). Atlas of the Night Sky. Collins. ISBN 978-0-00-717223-8.
- ^ 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, arXiv:1001.4289, Bibcode:2010MNRAS.404.1203F, doi:10.1111/j.1365-2966.2010.16373.x, S2CID 51825384.
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: CS1 maint: unflagged free DOI (link) - ^ Monthly Notices of the Royal Astronomical Society. nov 2016, published online aug 22 2016
External links
[edit]Media related to NGC 6101 at Wikimedia Commons