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http://hdl.handle.net/2248/5233
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DC Field | Value | Language |
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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 |
Appears in Collections: | IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
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High-resolution spectroscopy | 386.99 kB | Adobe PDF | View/Open |
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