A multicolour CCD photometric study of the open clusters NGC 2866, Pismis 19, Westerlund 2, ESO96-SC04, NGC 5617 and NGC 6204

被引:39
作者
Carraro, G
Munari, U
机构
[1] Univ Padua, Dipartimento Astron, I-35122 Padua, Italy
[2] Osserv Astron Padova, INAF, Sede Asiago, I-36012 Asiago, VI, Italy
关键词
stars : evolution; Hertzsprung-Russell (HR) diagram; open clusters and associations : general;
D O I
10.1111/j.1365-2966.2004.07244.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Accurate and deep BVI CCD photometry is presented for the core regions of six southern compact open clusters (supplemented in one case by U and R bands), which generally have only scanty photometric data published, in some cases only photoelectric or photographic. Together with adoption of modern reference isochrones, this has allowed us to derive improved values for their distance, reddening, age and main sequence morphology.
引用
收藏
页码:625 / 631
页数:7
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