Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5233
Title: High-resolution spectroscopy of the R Coronae Borealis and Other Hydrogen Deficient Stars
Authors: Kameswara Rao, N
Lambert, D. L
Issue Date: 2010
Publisher: Springer
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. 177-192
Series/Report no.: Astrophysics and Space Science Proceedings
Abstract: High-resolution spectroscopy is a very important tool for studying stellar physics, perhaps, particularly so for such enigmatic objects like the R Coronae Borealis and related Hydrogen deficient stars that produce carbon dust in addition to their peculiar abundances. Examples of how high-resolution spectroscopy is used in the study of these stars to address the two major puzzles are presented: (i) How are such rare H-deficient stars created? and (ii) How and where are the obscuring soot clouds produced around the R Coronae Borealis stars?
Description: The original publication is available at springerlink.com
URI: http://hdl.handle.net/2248/5233
???metadata.dc.rights???: © Springer
???metadata.dc.relation.uri???: http://www.springerlink.com/content/h248k73ll1500v88/
http://arxiv.org/abs/1002.3433
Appears in Collections:IIAP Publications

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