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

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

2010-02-18

arxiv.org/abs/1002.3433v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

16 pages, 9 figures, Astrophysics and Space Science Proceedings, Springer-Verlag, Berlin, 2010

Scientific paper

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?

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