THE ACS SURVEY OF GALACTIC GLOBULAR CLUSTERS. VI. NGC 6366: A HEAVILY STRIPPED GALACTIC GLOBULAR CLUSTER

被引:22
|
作者
Paust, Nathaniel E. Q. [1 ]
Aparicio, Antonio [2 ,3 ]
Piotto, Giampaolo [4 ]
Reid, I. Neill [1 ]
Anderson, Jay [1 ]
Sarajedini, Ata [5 ]
Bedin, Luigi R. [1 ]
Chaboyer, Brian [6 ]
Dotter, Aaron [6 ]
Hempel, Maren [5 ]
Majewski, Steven [7 ]
Marin-Franch, A. [8 ]
Milone, Antonino [4 ]
Rosenberg, Alfred [8 ]
Siegel, Michael [9 ]
机构
[1] Space Telescope Sci Inst, Baltimore, MD 21218 USA
[2] Univ La Laguna, Dept Astrophys, E-38200 San Cristobal la Laguna, Spain
[3] Inst Astrofis Canarias, E-38200 San Cristobal la Laguna, Spain
[4] Univ Padua, Dipartimento Astron, I-35122 Padua, Italy
[5] Univ Florida, Dept Astron, Gainesville, FL 32611 USA
[6] Dartmouth Coll, Dept Phys & Astron, Hanover, NH 03755 USA
[7] Univ Virginia, Dept Astron, Charlottesville, VA 22904 USA
[8] Inst Astrofis Canarias, E-38200 San Cristobal la Laguna, Spain
[9] Univ Texas Austin, McDonald Observ, Austin, TX 78712 USA
来源
ASTRONOMICAL JOURNAL | 2009年 / 137卷 / 01期
关键词
galaxies: luminosity function; mass function; globular clusters: general; globular clusters: individual (NGC 6366); COLOR-MAGNITUDE DIAGRAM; LOWER MAIN-SEQUENCE; LUMINOSITY FUNCTION; MASS FUNCTION; STELLAR POPULATION; ADVANCED CAMERA; STARS; CATALOG; SYSTEM; ISOCHRONES;
D O I
10.1088/0004-6256/137/1/246
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have used observations obtained as part of the Hubble Space Telescope/ACS Survey of Galactic globular clusters (GCs) to construct a color-magnitude diagram for the bulge cluster, NGC 6366. The luminosity function derived from those data extends to M-F606W similar to 9, or masses of similar to 0.3 M-circle dot. Unlike most GCs, the mass function peaks near the main-sequence turnoff with significantly fewer low-mass stars even after correction for completeness and mass segregation. Using a multimass King model, we extrapolate the global cluster behavior and find the global mass function to be poorly matched by a power law, with a particular deficit of stars with masses between 0.5 and 0.7 M-circle dot. We briefly discuss this interesting anomaly within the context of tidal stripping.
引用
收藏
页码:246 / 256
页数:11
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