A publishing partnership

Fluorine in R Coronae Borealis Stars

, , and

© 2008. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Gajendra Pandey et al 2008 ApJ 674 1068 DOI 10.1086/526492

0004-637X/674/2/1068

Abstract

Neutral fluorine (F I) lines are identified in the optical spectra of several R Coronae Borealis stars (RCBs) at maximum light. These lines provide the first measurement of the fluorine abundance in these stars. Fluorine is enriched in some RCBs by factors of 800-8000 relative to its likely initial abundance. The overabundances of fluorine are evidence for the synthesis of fluorine. These results are discussed in the light of the scenario that RCBs are formed by accretion of an He white dwarf by a C-O white dwarf. Sakurai's object (V4334 Sgr), a final He-shell flash product, shows no detectable F I lines.

Export citation and abstract BibTeX RIS

Please wait… references are loading.
10.1086/526492