Star formation in young cluster NGC 1893

Sharma, S; Pandey, A. K; Ojha, D. K; Chen, W. P; Ghosh, S. K; Bhatt, B. C; Maheswar, G; Sagar, R

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dc.contributor.author	Sharma, S
dc.contributor.author	Pandey, A. K
dc.contributor.author	Ojha, D. K
dc.contributor.author	Chen, W. P
dc.contributor.author	Ghosh, S. K
dc.contributor.author	Bhatt, B. C
dc.contributor.author	Maheswar, G
dc.contributor.author	Sagar, R
dc.date.accessioned	2009-09-14T16:21:24Z
dc.date.available	2009-09-14T16:21:24Z
dc.date.issued	2008-05
dc.identifier.citation	Vesperini, E., Giersz, Mirek and Sills, Alison. eds., Dynamical evolution of dense stellar systems., Proceedings of the 246th Symposium of the International Astronomical Union held in Capri, Italy, September 5 - 9, 2007, pp. 73 - 74	en
dc.identifier.isbn	978-0-521-87468-7
dc.identifier.issn	1743-9213
dc.identifier.uri	http://hdl.handle.net/2248/4819
dc.description	Open Access
dc.description.abstract	We have carried out a multi-wavelength study of the star forming region NGC 1893 to make a comprehensive exploration of the effects of massive stars on low mass star formation. Using deep optical U BV RI broad band, Hα narrow band photometry and slit-less spectroscopy along with archival data from the surveys such as 2MASS, MSX, IRAS and NVSS, we have studied the region to understand the star formation scenario in the region.	en
dc.language.iso	en	en
dc.publisher	International Astronomical Union	en
dc.relation.ispartofseries	IAU Symposium Proceedings Series;Vol. 246
dc.relation.uri	http://dx.doi.org/10.1017/S1743921308015342	en
dc.rights	© International Astronomical Union	en
dc.subject	Techniques: Photometric	en
dc.subject	Stars: Formation	en
dc.subject	Stars: Luminosity Function	en
dc.subject	Stars:Mass Function	en
dc.subject	Stars: Pre–Main-Sequence	en
dc.title	Star formation in young cluster NGC 1893	en
dc.type	Article	en