Spectrum variability of 25 Sextantis

dc.contributor.author	Rajamohan, R
dc.contributor.author	Paranjpye, A
dc.contributor.author	Sajeev, T. P
dc.date.accessioned	2009-02-04T16:15:11Z
dc.date.available	2009-02-04T16:15:11Z
dc.date.issued	1990-03
dc.identifier.citation	Astrophysics and Space Science, Vol. 165, No. 2, pp. 225 - 230	en
dc.identifier.issn	0004-640X
dc.identifier.uri	http://hdl.handle.net/2248/4327
dc.description.abstract	The identification of moderately strong spectral lines at a dispersion of 30 A per millimeter is given for the peculiar star 25 Sextantis. The observed variability of some of the lines are briefly described. It is found that lines of Fe I and Fe II are highly variable.	en
dc.language.iso	en	en
dc.publisher	Kluwer Academic Publishers	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1990Ap%26SS.165..225R	en
dc.relation.uri	http://dx.doi.org/10.1007/BF00653291	en
dc.subject	Spectral Line Width	en
dc.subject	Stellar Spectra	en
dc.subject	Variable Stars	en
dc.subject	Metallic Stars	en
dc.subject	Peculiar Stars	en
dc.title	Spectrum variability of 25 Sextantis	en
dc.type	Article	en