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Star Formation in Young Cluster NGC 1893

Published online by Cambridge University Press:  01 September 2007

Saurabh Sharma ,
A. K. Pandey ,
D. K. Ojha ,
W. P. Chen ,
S. K. Ghosh ,
B. C. Bhatt ,
G. Maheswar  and
Ram Sagar
Saurabh Sharma
Affiliation:
Aryabhatta Research Institute of Observational Sciences (ARIES), Nainital, 263 129, India; [email protected]
A. K. Pandey
Affiliation:
Aryabhatta Research Institute of Observational Sciences (ARIES), Nainital, 263 129, India; [email protected] Institute of Astronomy, National Central University, Chung-Li 32054, Taiwan
D. K. Ojha
Affiliation:
Tata Institute of Fundamental Research, Mumbai (Bombay) – 400 005, India
W. P. Chen
Affiliation:
Institute of Astronomy, National Central University, Chung-Li 32054, Taiwan
S. K. Ghosh
Affiliation:
Tata Institute of Fundamental Research, Mumbai (Bombay) – 400 005, India
B. C. Bhatt
Affiliation:
CREST, Indian Institute of Astrophysics, Hosakote 562 114, India
G. Maheswar
Affiliation:
Aryabhatta Research Institute of Observational Sciences (ARIES), Nainital, 263 129, India; [email protected]
Ram Sagar
Affiliation:
Aryabhatta Research Institute of Observational Sciences (ARIES), Nainital, 263 129, India; [email protected]
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Abstract

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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.

Keywords

techniques: photometricstars: formationstars: luminosity functionmass functionstars: pre–main-sequence
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S246: Dynamical Evolution of Dense Stellar Systems , September 2007 , pp. 73 - 74
Copyright
Copyright © International Astronomical Union 2008

References

Gaze, V. F. & Shajn, G. A., 1952, Izv. Krym. Astrofiz. Obs., 9, 52Google Scholar
Lada, E. A., Evans, N. J. II, Depoy, D. L., & Gatley, I., 1991, ApJ, 371, 171CrossRefGoogle Scholar
Lada, E. A. & Lada, C. J., 1995, AJ, 109, 1682CrossRefGoogle Scholar
Lada, C. J. & Lada, E. A., 2003, ARA&A, 41, 57Google Scholar
Marco, A. & Negueruela, I., 2002, A&A, 393, 195Google Scholar
Massey, P., Johnson, K. E., & DeGioia-Eastwood, K., 1995, ApJ, 454, 151CrossRefGoogle Scholar