Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7034
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dc.contributor.authorParthasarathy, M-
dc.date.accessioned2020-11-17T02:34:27Z-
dc.date.available2020-11-17T02:34:27Z-
dc.date.issued2017-02-
dc.identifier.citationNew Astronomy, Vol. 51, pp. 96-98en_US
dc.identifier.issn1384-1076-
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/7034-
dc.descriptionRestricted Access © Elsevier B.V http://dx.doi.org/10.1016/j.newast.2016.08.018en_US
dc.description.abstractThe discovery of K I 7699 Å line strength variations during the 1982–1984 eclipse of ε Aurigae is described. The equivalent widths and radial velocities of the K I 7699 Å line derived from spectra obtained during 1981 November–1983 July with the 2.1 m Otto Struve reflector telescope of the McDonald observatory are presenteden_US
dc.language.isoenen_US
dc.publisherElsevier B.Ven_US
dc.subjectStars: individual - ε Aurigaeen_US
dc.subjectStars: evolutionen_US
dc.subjectStars: circumstellar matteren_US
dc.subjectStars: eclipsing binariesen_US
dc.subjectStars: AGB and post-AGBen_US
dc.titleOn the discovery of K I 7699 Å line strength variation during the 1982–1984 eclipse of ε Aurigaeen_US
dc.typeArticleen_US
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