An improved Technique to Explore Disk Accretion Process in PMS Stars

dc.contributor.author	Parihar, P. S
dc.date.accessioned	2010-08-20T11:05:58Z
dc.date.available	2010-08-20T11:05:58Z
dc.date.issued	2010
dc.identifier.citation	Chaudhuri, R. K., Mekkaden, M. V., Raveendran, A. V & Narayanan, A. S., eds., Recent Advances In Spectroscopy: Theoretical, Astrophysical And Experimental Perspectives, Proceedings of the International Conference on Recent Advances in Spectroscopy - Theoretical, Astrophysical and Experimental Perspectives, Jan 28-31, 2009, Indian Institute of Astrophysics, Kodaikanal Observatory, Bangalore, India, pp. 223-228	en
dc.identifier.uri	http://hdl.handle.net/2248/5225
dc.description	The original publication is available at springerlink.com	en
dc.description.abstract	The low mass PMS stars are found to be surrounded by thick, flared accretion disk and the disk material is supposed to be funneled onto the stellar surface by strong and predominately dipolar magnetic field. We have developed a simple technique which uses medium resolution optical spectrum and gives reliable disk accretion rate. In this paper, we briefly describe the technique and also present the preliminary results obtained.	en
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.ispartofseries	Astrophysics and Space Science Proceedings
dc.relation.uri	http://www.springerlink.com/content/q31237254q581521/	en
dc.rights	© Springer	en
dc.title	An improved Technique to Explore Disk Accretion Process in PMS Stars	en
dc.type	Article	en