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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5225
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dc.contributor.authorParihar, P. S-
dc.date.accessioned2010-08-20T11:05:58Z-
dc.date.available2010-08-20T11:05:58Z-
dc.date.issued2010-
dc.identifier.citationChaudhuri, 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. 223-228en
dc.identifier.urihttp://hdl.handle.net/2248/5225-
dc.descriptionThe original publication is available at springerlink.comen
dc.description.abstractThe 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.isoenen
dc.publisherSpringeren
dc.relation.ispartofseriesAstrophysics and Space Science Proceedings-
dc.relation.urihttp://www.springerlink.com/content/q31237254q581521/en
dc.rights© Springeren
dc.titleAn improved Technique to Explore Disk Accretion Process in PMS Starsen
dc.typeArticleen
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