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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2638
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dc.contributor.authorSaraswat, P-
dc.contributor.authorApparao, K. M. V-
dc.date.accessioned2008-07-11T10:21:46Z-
dc.date.available2008-07-11T10:21:46Z-
dc.date.issued1994-
dc.identifier.citationIAU Symposium, No. 162, pp. 213 – 215en
dc.identifier.issn0074-1809-
dc.identifier.urihttp://hdl.handle.net/2248/2638-
dc.format.extent293881 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherInternational Astronomical Unionen
dc.relation.urihttp://adsabs.harvard.edu/abs/1994IAUS..162..213Sen
dc.subjectStar disk structureen
dc.subjectX-ray observationsen
dc.subjectStellar wind modelen
dc.subject4U1907+09en
dc.titleBe star disk structure as implied by X-ray observationsen
dc.typeArticleen
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