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PFLEIDERER 2: IDENTIFICATION OF A NEW GLOBULAR CLUSTER IN THE GALAXY

Journal Article · · Astronomical Journal (New York, N.Y. Online)
 [1]; ;  [2]
  1. Universita di Padova, Dipartimento di Astronomia, Vicolo dell'Osservatorio 5, I-35122 Padova (Italy)
  2. Universidade Federal do Rio Grande do Sul, Departamento de Astronomia, CP 15051, Porto Alegre 91501-970 (Brazil)
We provide evidence that indicates the star cluster Pfleiderer 2, which is projected in a rich field, as a newly identified Galactic globular cluster. Since it is located in a crowded field, core extraction and decontamination tools were applied to reveal the cluster sequences in B, V, and I color-magnitude diagrams (CMDs). The main CMD features of Pfleiderer 2 are a tilted red giant branch and a red horizontal branch, indicating a high metallicity around solar. The reddening is E(B - V) = 1.01. The globular cluster is located at a distance of d {sub sun} = 16 {+-} 2 kpc from the Sun. The cluster is located 2.7 kpc above the Galactic plane and at a distance of R {sub GC} = 9.7 kpc from the Galactic center, which is unusual for a metal-rich globular cluster.
OSTI ID:
21301629
Journal Information:
Astronomical Journal (New York, N.Y. Online), Journal Name: Astronomical Journal (New York, N.Y. Online) Journal Issue: 3 Vol. 138; ISSN 1538-3881
Country of Publication:
United States
Language:
English

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