Star Formation in Young Cluster NGC 1893

Details Star Formation in Young Cluster NGC 1893 Star Formation in Young Cluster NGC 1893

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008iaus..246...73s&link_type=abstract

Dynamical Evolution of Dense Stellar Systems, Proceedings of the International Astronomical Union, IAU Symposium, Volume 246, p.

Astronomy and Astrophysics

Astronomy

Techniques: Photometric, Stars: Formation, Stars: Luminosity Function, Mass Function, Stars: Pre–Main-Sequence

Scientific paper

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.

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