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Abundance similarities between the R CrB star V854 Cen and the born-again Sakurai's object
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Faculty of Science and Technology, Astronomical observatory.
1998 (English)In: ASTRONOMY AND ASTROPHYSICS, ISSN 0004-6361, Vol. 332, no 2, 651-660 p.Article in journal (Refereed) Published
Abstract [en]

The elemental abundances of the mildly hydrogen-deficient R Coronae Borealis (R CrB) star V854 Cen have been estimated. The R CrB stars have been divided into majority and minority classes judging by their abundance patterns. Class assignment has previous

Place, publisher, year, edition, pages
SPRINGER VERLAG , 1998. Vol. 332, no 2, 651-660 p.
Keyword [en]
stars : individual : V854 Cen; stars : variables : R Coronae Borealis; stars : abundances; stars : AGB and post-AGB; stars : evolution; stars : individual : Sakurai's object; CORONAE-BOREALIS STARS; OPACITY CALCULATIONS; HEAVY-ELEMENTS; ATOMIC DATA; MERE
National Category
Astronomy, Astrophysics and Cosmology
URN: urn:nbn:se:uu:diva-85317OAI: oai:DiVA.org:uu-85317DiVA: diva2:113225
Addresses: Asplund M, Astron Observ, Box 515, S-75120 Uppsala, Sweden. Astron Observ, S-75120 Uppsala, Sweden. Indian Inst Astrophys, Bangalore 560034, Karnataka, India. Univ Texas, Dept Astron, Austin, TX 78712 USA.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-14

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