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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4819
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dc.contributor.authorSharma, S-
dc.contributor.authorPandey, A. K-
dc.contributor.authorOjha, D. K-
dc.contributor.authorChen, W. P-
dc.contributor.authorGhosh, S. K-
dc.contributor.authorBhatt, B. C-
dc.contributor.authorMaheswar, G-
dc.contributor.authorSagar, R-
dc.date.accessioned2009-09-14T16:21:24Z-
dc.date.available2009-09-14T16:21:24Z-
dc.date.issued2008-05-
dc.identifier.citationVesperini, 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 - 74en
dc.identifier.isbn978-0-521-87468-7-
dc.identifier.issn1743-9213-
dc.identifier.urihttp://hdl.handle.net/2248/4819-
dc.descriptionOpen Access-
dc.description.abstractWe 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.isoenen
dc.publisherInternational Astronomical Unionen
dc.relation.ispartofseriesIAU Symposium Proceedings Series;Vol. 246-
dc.relation.urihttp://dx.doi.org/10.1017/S1743921308015342en
dc.rights© International Astronomical Unionen
dc.subjectTechniques: Photometricen
dc.subjectStars: Formationen
dc.subjectStars: Luminosity Functionen
dc.subjectStars:Mass Functionen
dc.subjectStars: Pre–Main-Sequenceen
dc.titleStar formation in young cluster NGC 1893en
dc.typeArticleen
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