Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/26543
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dc.contributor.authorNayakshin, S-
dc.contributor.authorKazanas, D-
dc.contributor.authorKallman, TR-
dc.date.accessioned2012-10-24T09:21:50Z-
dc.date.available2012-10-24T09:21:50Z-
dc.date.issued2000-7-10-
dc.identifier.citationASTROPHYSICAL JOURNAL, 2000, 537 (2), pp. 833-852-
dc.identifier.issn0004-637X-
dc.identifier.urihttp://hdl.handle.net/2381/26543-
dc.formatmetadata-
dc.language.isoEnglish-
dc.publisherUNIV CHICAGO PRESS-
dc.sourceWeb of Science-
dc.source.urihttp://webofknowledge.com-
dc.subjectScience & Technology-
dc.subjectPhysical Sciences-
dc.subjectAstronomy & Astrophysics-
dc.subjectaccretion-
dc.subjectaccretion disks-
dc.subjectline : formation-
dc.subjectradiation mechanisms : nonthermal radiative transfer-
dc.subjectX-rays : general-
dc.subjectACTIVE GALACTIC NUCLEI-
dc.subjectVERTICAL STRUCTURE-
dc.subjectSEYFERT-GALAXIES-
dc.subjectCOLD MATTER-
dc.subjectCOMPTON REFLECTION-
dc.subjectBINARY-SYSTEM-
dc.subjectMASS-TRANSFER-
dc.subjectBLACK-HOLES-
dc.subjectEMISSION-
dc.subjectCORONAE-
dc.titleThermal instability and photoionized X-ray reflection in accretion disks-
dc.typeJournal Article-
dc.identifier.doi10.1086/309054-
dc.description.irispid9277-
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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