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The R Coronae Borealis stars - atmospheres and abundances
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics.
2000 (English)In: ASTRONOMY AND ASTROPHYSICS, ISSN 0004-6361, Vol. 353, no 1, 287-310 p.Article in journal (Refereed) Published
Abstract [en]

An abundance analysis of the H-deficient and He- and C-rich R Coronae Borealis (R CrB) stars has been undertaken to examine the ancestry of the stars. The investigation is based on high-resolution spectra and line-blanketed H-deficient model atmospheres.

Place, publisher, year, edition, pages
SPRINGER VERLAG , 2000. Vol. 353, no 1, 287-310 p.
Keyword [en]
stars : abundances; stars : evolution; stars : AGB and post-AGB; stars : variables : general; stars : individual : RCrB; stars : individual : Sakurai's object; EXTREME HELIUM STARS; HIGH-RESOLUTION SPECTROSCOPY; DEFICIENT CARBON STARS; MODEL ATMOSPHERES;
URN: urn:nbn:se:uu:diva-36616OAI: oai:DiVA.org:uu-36616DiVA: diva2:64515
Addresses: Asplund M, NORDITA, Blegdamsvej 17, DK-2100 Copenhagen O, Denmark. NORDITA, DK-2100 Copenhagen O, Denmark. Astron Observ, S-75120 Uppsala, Sweden. Univ Texas, Dept Astron, Austin, TX 78712 USA. Indian Inst Astrophys, Bangalore 560034, KarnatakaAvailable from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-14

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