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dc.contributor.authorDrew, J.E.
dc.contributor.authorDenby, M.
dc.contributor.authorHoare, M.G.
dc.date.accessioned2009-12-01T15:03:23Z
dc.date.available2009-12-01T15:03:23Z
dc.date.issued1994
dc.identifier.citationDrew , J E , Denby , M & Hoare , M G 1994 , ' Soft x-ray observations of the early b-giants beta and epsilon CMA ' Monthly Notices of the Royal Astronomical Society , vol 266 , no. 4 , pp. 917-924 .
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 155140
dc.identifier.otherPURE UUID: 9b7e6e9c-5847-440c-bd90-aab59decc582
dc.identifier.otherdspace: 2299/4050
dc.identifier.urihttp://hdl.handle.net/2299/4050
dc.descriptionOriginal article can be found at: http://adsabs.harvard.edu/basic_search.html Copyright Royal Astronomical Society [Full text of this article is not available in the UHRA]
dc.description.abstractThe study reports observations performed with the PSPC on board the Roentgensatellit (ROSAT) of the two nearby giant stars Beta CMa (B1 II-III) and Epsilon CMa (B2 II). Upper limits in the region of +/- 10 percent can be set on the variation of the 0.1-0.4 keV and 0.5-2.0 keV fluxes from Beta CMa. By attributing the soft X-ray emission to an outer zone of hot shocked gas enclosing the cool inner wind responsible for observed UV blueshifted absorption features, it is estimated that the mass loss for Beta and Epsilon CMa, respectively, are (6 +/- 2) x 10 exp 9 and (8 +/- 2) x 10 exp -9 solar mass/yr.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleSoft x-ray observations of the early b-giants beta and epsilon CMAen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstyperestrictedAccess


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