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1.11. A photometric study of two galactic bulge globular clusters

Published online by Cambridge University Press:  25 May 2016

Myung Gyoon Lee ,
Soung Chul Yang ,
Jeong Hoon Yang  and
Doug Geisler
Myung Gyoon Lee
Affiliation:
Department of Astronomy, Seoul Naional University, Korea
Soung Chul Yang
Affiliation:
Department of Astronomy, Seoul Naional University, Korea
Jeong Hoon Yang
Affiliation:
Department of Astronomy, Seoul Naional University, Korea
Doug Geisler
Affiliation:
NOAO/KPNO, Tucson, Arizona, USA

Extract

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We present a comparative study of two metal-rich globular clusters in the Galactic bulge, NGC 6316 and NGC 6624, based on Washington CCD photometry. These two clusters are very close to the Galactic center. NGC 6624 is known to be dynamically in a post-core-collapse stage, while NGC 6316 is not. CMT1T2 CCD images of these clusters were obtained at the CTIO 0.9m telescope. We adopt the reddening values of E(B – V) = 0.61 for NGC 6316 and E(B – V) = 0.26 for NGC 6624 in this study.

Type
Part I. Stellar Cluster, Star Formation
Information
Symposium - International Astronomical Union , Volume 184: The Central Regions of the Galaxy and Galaxies , 1998 , pp. 37 - 38
Copyright
Copyright © Kluwer 1998