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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4336
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dc.contributor.authorRosario, M. J-
dc.contributor.authorMekkaden, M. V-
dc.contributor.authorRaveendran, A. V-
dc.date.accessioned2009-02-05T11:26:20Z-
dc.date.available2009-02-05T11:26:20Z-
dc.date.issued2008-06-
dc.identifier.citationInformation Bulletin on Variable Stars, No. 5836, pp. 1 - 4en
dc.identifier.issn0374-0676-
dc.identifier.urihttp://hdl.handle.net/2248/4336-
dc.description.abstractWe present new BV photometry of UX Ari obtained on 23 nights during January-March 2008. From an analysis of the long-term V band photometry available for this star we find strong evidence for the orbital modulation of spot activity in the cool component of UX Ari: the hemisphere facing the companion shows a higher level of spot activity, as indicated by a significantly larger spread in observed brightness, when compared to that away from it.en
dc.language.isoenen
dc.publisherKonkoly Observatoryen
dc.relation.urihttp://www.konkoly.hu/cgi-bin/IBVS?5836en
dc.rights© Konkoly Observatoryen
dc.subjectUX Arien
dc.subjectPhotometryen
dc.subjectAsymmetry in Spot Activityen
dc.subjectOrbital Reference Frameen
dc.titleUX Ari: new photometry and longitudinal asymmetry in spot activity fixed in orbital reference frameen
dc.typeArticleen
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