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  5. Ultra-deep GEMINI Near-infrared Observations of the Bulge Globular Cluster NGC 6624
 

Ultra-deep GEMINI Near-infrared Observations of the Bulge Globular Cluster NGC 6624

Journal
THE ASTROPHYSICAL JOURNAL  
Date Issued
2016
Author(s)
Saracino, S.
•
Dalessandro, Emanuele  
•
Ferraro, F. R.
•
Geisler, D.
•
Mauro, F.
•
Lanzoni, B.
•
ORIGLIA, Livia  
•
Miocchi, P.
•
Cohen, R. E.
•
Villanova, S.
•
Moni Bidin, C.
DOI
10.3847/0004-637X/832/1/48
Abstract
We used ultra-deep J and K s images secured with the near-infrared (NIR) GSAOI camera assisted by the multi-conjugate adaptive optics system GeMS at the GEMINI South Telescope in Chile, to obtain a (K s , J - K s ) color-magnitude diagram (CMD) for the bulge globular cluster NGC 6624. We obtained the deepest and most accurate NIR CMD from the ground for this cluster, by reaching K s ∼ 21.5, approximately 8 mag below the horizontal branch level. The entire extension of the Main Sequence (MS) is nicely sampled and at K s ∼ 20 we detected the so-called MS “knee” in a purely NIR CMD. By taking advantage of the exquisite quality of the data, we estimated the absolute age of NGC 6624 (t age = 12.0 ± 0.5 Gyr), which turns out to be in good agreement with previous studies in the literature. We also analyzed the luminosity and mass functions of MS stars down to M ∼ 0.45 M☉, finding evidence of a significant increase of low-mass stars at increasing distances from the cluster center. This is a clear signature of mass segregation, confirming that NGC 6624 is in an advanced stage of dynamical evolution.

Based on observations obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), Ministério da Ciência, Tecnologia e Inovação (Brazil) and Ministerio de Ciencia, Tecnología e Innovación Productiva (Argentina). Based on observations gathered with ESO-VISTA telescope (program ID 179.B-2002).

Volume
832
Issue
1
Start page
48
Uri
http://hdl.handle.net/20.500.12386/26228
Url
https://iopscience.iop.org/article/10.3847/0004-637X/832/1/48
Issn Identifier
0004-637X
Ads BibCode
2016ApJ...832...48S
Rights
open.access
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Saracino_2016_ApJ_832_48.pdf

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7.02 MB

Format

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Checksum (MD5)

6732738252986cfd473ec0e5c2af0a47

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