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An analysis of the atmosphere of T volupeculae

Show simple item record Rautela, B. B. 2010-08-20T08:11:18Z 2010-08-20T08:11:18Z 1981
dc.identifier.citation This article downloded from ADS Free Online Journal en_US
dc.description.abstract Ten spectrograms of T Vul at a dispersion of 8.47Å mm-¹ have been used for an analysis of the parameters of stellar atmosphere during its pulsation cycle. A differential curve of growth method relative to the Sun has been used to evaluate atmospheric parameters. The range in ɵexc is from 0.88 to 1.00. Mean abundances for twenty elements have been estimated relative to [N fe]. A deficiency by a factor of 2.4 has been found in S-process elements with respect to those formed by the e-process. en_US
dc.language.iso en_US en_US
dc.relation.ispartofseries ass77-369
dc.subject Atomospheric Science, Parameters of stellar atmosphere, Pulsation cycle, S-process elements, e-process en_US
dc.title An analysis of the atmosphere of T volupeculae en_US
dc.type Article en_US

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