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dc.contributor.author | Lipunova G. | |
dc.contributor.author | Suleimanov V. | |
dc.date.accessioned | 2018-09-17T21:32:33Z | |
dc.date.available | 2018-09-17T21:32:33Z | |
dc.date.issued | 2004 | |
dc.identifier.issn | 1392-0049 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/135127 | |
dc.description.abstract | We solve the vertical structure equations for a standard α-disk and compare the results with those obtained by an independent method (Ketsaris & Shakura 1998). On the basis of the numerical solutions for the vertical structure we obtain analytic radial dependences for the physical parameters of the disk. For a disk consisting of fully ionized hydrogen, its half-thickness is about 2.5 times larger than that obtained by the "standard" solution, averaging the vertical structure equations. Account of heavy elements leads to an additional increase of the half-thickness by approximately 25%. | |
dc.relation.ispartofseries | Baltic Astronomy | |
dc.subject | Accretion | |
dc.subject | Accretion disks | |
dc.title | Radial dependences of physical parameters in α-disk as a consequence of two vertical structure solutions | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 1 | |
dc.relation.ispartofseries-volume | 13 | |
dc.collection | Публикации сотрудников КФУ | |
dc.relation.startpage | 167 | |
dc.source.id | SCOPUS13920049-2004-13-1-SID24944530349 |