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


Autoria(s): ORTOLANI, S.; BONATTO, C.; BICA, E.; BARBUY, B.
Contribuinte(s)

UNIVERSIDADE DE SÃO PAULO

Data(s)

18/04/2012

18/04/2012

2009

Resumo

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(circle dot) = 16 +/- 2 kpc from the Sun. The cluster is located 2.7 kpc above the Galactic plane and at a distance of R(GC) = 9.7 kpc from the Galactic center, which is unusual for a metal-rich globular cluster.

CNPq

Fapesp

Ministero dell'Universita e della Ricerca Scientifica e Tecnologica (MURST), Italy

Identificador

ASTRONOMICAL JOURNAL, v.138, n.3, p.889-894, 2009

0004-6256

http://producao.usp.br/handle/BDPI/15703

10.1088/0004-6256/138/3/889

http://dx.doi.org/10.1088/0004-6256/138/3/889

Idioma(s)

eng

Publicador

IOP PUBLISHING LTD

Relação

Astronomical Journal

Direitos

closedAccess

Copyright IOP PUBLISHING LTD

Palavras-Chave #globular clusters: individual (Pfleiderer 2) #Hertzsprung-Russell (HR) diagram #PHOTOMETRIC STANDARD STARS #CELESTIAL EQUATOR #MILKY-WAY #CANDIDATES #CATALOG #Astronomy & Astrophysics
Tipo

article

original article

publishedVersion