A systematic survey for infrared star clusters with |b| < 20° using 2MASS

被引:166
作者
Froebrich, D.
Scholz, A.
Raftery, C. L.
机构
[1] Dublin Inst Adv Studies, Dublin 2, Ireland
[2] Univ Kent, Ctr Astrophys & Planetary Sci, Canterbury CT2 7NH, Kent, England
[3] Univ Toronto, Toronto, ON, Canada
[4] Trinity Coll Dublin, Dublin 2, Ireland
关键词
methods : statistical; globular clusters : general; open clusters and associations : general;
D O I
10.1111/j.1365-2966.2006.11148.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We used star density maps obtained from the Two-Micron All-Sky Survey (2MASS) to obtain a sample of star clusters in the entire Galactic Plane with vertical bar b vertical bar < 20 degrees. A total of 1788 star cluster candidates are identified in this survey. Among those are 681 previously known open clusters and 86 globular clusters. A statistical analysis indicates that our sample of 1021 new cluster candidates has a contamination of about 50 per cent. Star cluster parameters are obtained by fitting a King profile to the star density. These parameters are used to statistically identify probable new globular cluster candidates in our sample. A detailed investigation of the projected distribution of star clusters in the Galaxy demonstrates that they show a clear tendency to cluster on spatial scales in the order of 12-25 pc, a typical size for molecular clouds.
引用
收藏
页码:399 / 408
页数:10
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