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dc.contributor.authorJeffers, S V
dc.contributor.authorCameron, A C
dc.contributor.authorBarnes, J R
dc.contributor.authorAufdenberg, J P
dc.contributor.authorHussain, G A J
dc.contributor.editorFavata, F
dc.contributor.editorHussain, G A J
dc.contributor.editorBattrick, B
dc.date.accessioned2011-12-20T12:01:13Z
dc.date.available2011-12-20T12:01:13Z
dc.date.issued2005
dc.identifier.citationJeffers , S V , Cameron , A C , Barnes , J R , Aufdenberg , J P & Hussain , G A J 2005 , Dense spot coverage and polar caps on SV Cam . in F Favata , G A J Hussain & B Battrick (eds) , Procs of the 13th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun . European Space Agency , PARIS , pp. 669-671 , 13th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun , Hamburg , 5/07/04 .
dc.identifier.citationconference
dc.identifier.isbn92-9092-871-9
dc.identifier.otherPURE: 497144
dc.identifier.otherPURE UUID: 1b4d1345-85f5-418c-ab89-b0166b44891c
dc.identifier.otherWOS: 000231306900121
dc.identifier.otherScopus: 23844495522
dc.identifier.urihttp://hdl.handle.net/2299/7406
dc.description.abstractWe have used spectrophotometric data from 9 HST orbits to eclipse-map the primary component of the RS CVn binary SV Cam. From these observations and SV Cam's HIPPARCOS parallax we find that the surface flux in the eclipsed low-latitude region is about 30% lower than computed from the best fitting PHOENIX model atmosphere. The flux deficit can only be accounted for if about a third of the primary's surface is covered with unresolved spots. Even when we extend the spottedness from the eclipsed region to the entire surface, there still remains an unaccounted flux deficit. The remaining flux deficit is explained by the presence of a large polar spot extending down to latitude 48 +/- 6 degrees.en
dc.format.extent3
dc.language.isoeng
dc.publisherEuropean Space Agency
dc.relation.ispartofProcs of the 13th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun
dc.subjectstars : activity
dc.subjectstars : spots binaries : eclipsing
dc.subjectSTARS
dc.titleDense spot coverage and polar caps on SV Camen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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