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 |
|