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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 |
| Appears in Collections: | IIAP Publications |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| High-resolution spectroscopy | 386.99 kB | Adobe PDF | View/Open |
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