Deep optical and near infrared imaging photometry of the Serpens cloud core

被引：0
作者：
Giovannetti, P
Caux, E
Nadeau, D
Monin, JL
机构：
[1] Ctr Etud Spatiale Rayonnements, F-31028 Toulouse 04, France
[2] Univ Montreal, Dept Phys, Quebec City, PQ H3C 3J7, Canada
[3] Univ Montreal, Observ Mt Megant, Quebec City, PQ H3C 3J7, Canada
[4] Univ Grenoble 1, Observ Grenoble, Astrophys Lab, F-38041 Grenoble, France
来源：
ASTRONOMY & ASTROPHYSICS | 1998年 / 330卷 / 03期
关键词：
stars : pre-main sequence; ISM : open clusters : Serpens cloud; stars : luminosity function; infrared : stars; star formation;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present results from a deep optical (VRI) and near infrared (JHK) survey of the central part of the Serpens molecular cloud. A total of 138 sources were detected in the 19 arcmin(2) surveyed area down to a limiting magnitude of 16.3 in K. We find that the form of the observed K Luminosity Function (KLF) of stars belonging to the Serpens Molecular cloud is consistent with that predicted from a Miller & Scale (1979) Interstellar Mass Function (IMF). We have investigated the KLF evolution with the age of a cluster by modeling KLFs of hypothetical clusters. Our results suggest that two phases of star formation could have taken place in the Serpens core.
引用
收藏
页码：990 / 998
页数：9
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