High-resolution spectroscopy of the R Coronae Borealis and Other Hydrogen Deficient Stars

Kameswara Rao, N; Lambert, D. L

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dc.contributor.author	Kameswara Rao, N
dc.contributor.author	Lambert, D. L
dc.date.accessioned	2010-08-25T10:05:55Z
dc.date.available	2010-08-25T10:05:55Z
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. 177-192	en
dc.identifier.uri	http://hdl.handle.net/2248/5233
dc.description	The original publication is available at springerlink.com	en
dc.description.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?	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/h248k73ll1500v88/	en
dc.relation.uri	http://arxiv.org/abs/1002.3433	en
dc.rights	© Springer	en
dc.title	High-resolution spectroscopy of the R Coronae Borealis and Other Hydrogen Deficient Stars	en
dc.type	Article	en