An analysis of the atmosphere of T volupeculae

dc.contributor.author	Rautela, B. B.
dc.date.accessioned	2010-08-20T08:11:18Z
dc.date.available	2010-08-20T08:11:18Z
dc.date.issued	1981
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/741
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