Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/19675
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dc.contributor.authorKing, AR-
dc.contributor.authorKolb, U-
dc.contributor.authorBurderi, L-
dc.date.accessioned2012-10-24T09:07:29Z-
dc.date.available2012-10-24T09:07:29Z-
dc.date.issued1996-6-20-
dc.identifier.citationASTROPHYSICAL JOURNAL, 1996, 464 (2), pp. L127-L130-
dc.identifier.issn0004-637X-
dc.identifier.urihttp://hdl.handle.net/2381/19675-
dc.formatmetadata-
dc.language.isoEnglish-
dc.publisherIOP PUBLISHING LTD-
dc.sourceWeb of Science-
dc.source.urihttp://webofknowledge.com-
dc.subjectScience & Technology-
dc.subjectPhysical Sciences-
dc.subjectAstronomy & Astrophysics-
dc.subjectaccretion-
dc.subjectaccretion disks-
dc.subjectbinaries-
dc.subjectclose-
dc.subjectblack hole physics-
dc.subjectinstabilities-
dc.subjectMASS-
dc.subjectEVOLUTION-
dc.subjectSYSTEMS-
dc.titleBlack hole binaries and X-ray transients-
dc.typeJournal Article-
dc.identifier.doi10.1086/310105-
dc.description.irispid45427-
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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