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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2573
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dc.contributor.authorKameswara Rao, N-
dc.contributor.authorGilra, D. P-
dc.date.accessioned2008-07-02T09:31:16Z-
dc.date.available2008-07-02T09:31:16Z-
dc.date.issued1983-03-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 4, No. 1, pp. 59 – 63en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/2573-
dc.descriptionOpen Access-
dc.description.abstractIUE observations of HD 62001 do not confirm the ultraviolet variability of 0.15 mag seen from the ANS observations. These intriguing variations in ANS observations seem to be caused by a nearby (∼ 70 arcsec away) B star getting in and out of the field of view of the telescope, which had a jitter of 20 arcsec. There seems to be no evidence for the presence of a hot companion, either from the energy distribution or from UV variability. However, visual light variations are present. This, coupled with the radial velocity variations, indicates a binary nature probably of Algol type.en
dc.format.extent805603 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://adsabs.harvard.edu/abs/1983JApA....4...59Ren
dc.relation.urihttp://www.springerlink.com/content/82l2516167t20l8t/-
dc.subjectVariable Starsen
dc.subjectPhotometryen
dc.subjectUltraviolet Spectroscopyen
dc.titleUltraviolet variability of HD 62001 - The central star of the missing nebula V-V 1-7en
dc.typeArticleen
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