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Palomar 12
Globular cluster in the constellation Capricornus
Globular cluster in the constellation Capricornus
Palomar 12 is a globular cluster in the constellation Capricornus, and is a member of the Palomar Globular Clusters group.
First discovered on the National Geographic Society – Palomar Observatory Sky Survey plates by Robert George Harrington and Fritz Zwicky,{{cite journal | author-link = George Ogden Abell | doi-access=free it was initially catalogued as a globular cluster; however, Zwicky came to believe it was actually a nearby dwarf galaxy in the Local Group. It is a relatively young cluster, being about 30% younger than most of the globular clusters in the Milky Way. It is metal-rich with a metallicity of . It has an average luminosity distribution of .{{Cite journal | author-link1 = Sidney van den Bergh
Based on proper motion studies, this cluster was first suspected in 2000 to have been captured from the Sagittarius Dwarf Elliptical Galaxy (SagDEG) about 1.7 Ga ago.{{cite journal
References
References
- distance × sin( diameter_angle / 2 ) = 162 ly. radius
- (December 2010). "The ACS Survey of Galactic Globular Clusters. X. New Determinations of Centers for 65 Clusters". The Astronomical Journal.
- "Cl Pal 12".
- (1998). "Young Galactic globular clusters II. The case of Palomar 12". Astronomy and Astrophysics.
- (September 2007). "Chemical Abundances and Kinematics in Globular Clusters and Local Group Dwarf Galaxies and Their Implications for Formation Theories of the Galactic Halo". The Publications of the Astronomical Society of the Pacific.
- (November 2011). "Young Radio Pulsars in Galactic Globular Clusters". The Astrophysical Journal.
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