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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4327
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dc.contributor.authorRajamohan, R-
dc.contributor.authorParanjpye, A-
dc.contributor.authorSajeev, T. P-
dc.date.accessioned2009-02-04T16:15:11Z-
dc.date.available2009-02-04T16:15:11Z-
dc.date.issued1990-03-
dc.identifier.citationAstrophysics and Space Science, Vol. 165, No. 2, pp. 225 - 230en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2248/4327-
dc.description.abstractThe 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.isoenen
dc.publisherKluwer Academic Publishersen
dc.relation.urihttp://adsabs.harvard.edu/abs/1990Ap%26SS.165..225Ren
dc.relation.urihttp://dx.doi.org/10.1007/BF00653291en
dc.subjectSpectral Line Widthen
dc.subjectStellar Spectraen
dc.subjectVariable Starsen
dc.subjectMetallic Starsen
dc.subjectPeculiar Starsen
dc.titleSpectrum variability of 25 Sextantisen
dc.typeArticleen
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