Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5996
Title: Duration of star formation in young open clusters
Authors: Bhavya, B
Subramaniam, A
Kuriakose, V. C
Keywords: Stars;Formation -- stars;Pre-main sequence -- (Galaxy);Open clusters and associations general
Issue Date: 2012
Publisher: Astronomical Society of India
Citation: ASI Conference Series, Vol. 4, pp. 121-124
Abstract: Young Open Clusters have always been a platform for the star formation studies. It was assumed that all members in the cluster are coeval, on the other hand, recent studies show the presence of an age range among the members of young open clusters. Presence of pre-main sequence (PMS) stars are identified by combining optical and near-IR data for 13 young clusters. Age-wise and mass-wise distribution of PMS stars are analysed to study how star formation proceeded in the clusters. In all the clusters we studied, we find an age range among the PMS stars and the duration of star formation is found to be similar to the cluster age.
Description: Open Access
URI: http://hdl.handle.net/2248/5996
ISBN: 978-81-922926-2-5
???metadata.dc.rights???: © Astronomical Society of India
???metadata.dc.relation.uri???: http://www.ncra.tifr.res.in:8081/~basi/ASICS_4/Abstracts/bhavya.html
Appears in Collections:IIAP Publications

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