Abstract:
We present results on the age and metallicity estimates of the astonishingly unstudied Small Magellanic Cloud (SMC) cluster (ESO51-SC09), from CCD BVI photometry obtained at the ESO NTT with the EMMI attached. ESO51-SC09 turns out to be a relatively small cluster (FWHM = 10± 1pc) located ∼4° northward from the galaxy center. We report for the first time a mean cluster age of 7.0± 1.3Gyr and a mean cluster metallicity of [Fe/H]= -1.00± 0.15dex, concluding that ESO51-SC09 belongs to the group of the oldest SMC clusters. We found that the cluster is projected onto an older (age ∼10-13Gyr) and more metal-poor ([Fe/H]= -1.3± 0.2dex) dominant field stellar population, so that the cluster could have reached its current location because of its orbital motion. © 2012 The American Astronomical Society. All rights reserved.
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Citas:
---------- APA ----------
(2012)
. Identification of a new relatively old star cluster in the small magellanic cloud. Astrophysical Journal Letters, 756(2).
http://dx.doi.org/10.1088/2041-8205/756/2/L32---------- CHICAGO ----------
Piatti, A.E.
"Identification of a new relatively old star cluster in the small magellanic cloud"
. Astrophysical Journal Letters 756, no. 2
(2012).
http://dx.doi.org/10.1088/2041-8205/756/2/L32---------- MLA ----------
Piatti, A.E.
"Identification of a new relatively old star cluster in the small magellanic cloud"
. Astrophysical Journal Letters, vol. 756, no. 2, 2012.
http://dx.doi.org/10.1088/2041-8205/756/2/L32---------- VANCOUVER ----------
Piatti, A.E. Identification of a new relatively old star cluster in the small magellanic cloud. Astrophys. J. Lett. 2012;756(2).
http://dx.doi.org/10.1088/2041-8205/756/2/L32