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The stability of late-type stars close to the Eddington limit
Uppsala University.
1998 (English)In: ASTRONOMY AND ASTROPHYSICS, ISSN 0004-6361, Vol. 330, no 2, 641-650 p.Article in journal (Other scientific) Published
Abstract [en]

The opacity-modified Eddington limit has been computed for hydrogen-deficient model atmospheres. The R Coronae Borealis (R CrB) stars are found to be located strikingly close to the limit, which suggests that the unknown trigger mechanism for their visual

Place, publisher, year, edition, pages
SPRINGER VERLAG , 1998. Vol. 330, no 2, 641-650 p.
Keyword [en]
stars : model atmospheres; instabilities; stars : AGB and post-AGB; stars : mass-loss; stars : evolution; stars variables : R Coronae Borealis; stars : variables : Luminous Blue Variables; LUMINOUS BLUE VARIABLES; ATMOSPHERES; INSTABILITY
URN: urn:nbn:se:uu:diva-85326OAI: oai:DiVA.org:uu-85326DiVA: diva2:113234
Addresses: Asplund M, NORDITA, Blegdamsvej 17, DK-2100 Copenhagen 0, Denmark. Astron Observ, S-75120 Uppsala, Sweden.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-14

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