dc.contributor.author |
Srinivasa Rao, M |
|
dc.date.accessioned |
2006-04-08T05:35:25Z |
|
dc.date.available |
2006-04-08T05:35:25Z |
|
dc.date.issued |
2009 |
|
dc.identifier.citation |
Publications of the Astronomical Observatory of Belgrade, Vol. 86, pp. 59-66 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/874 |
|
dc.description.abstract |
A concise description of the method of obtaining the solution of radiative trans-
fer equation which can be applied to di®erent geometrical and physical systems is given.
This paper mainly deals with the steps for obtaining solution of transfer equation like (1)
interaction principle for di®erent geometries, (2) star product and (3) calculation of radiation
field at internal points, and their applications in stellar atmosphere problems; in particular
(a) study of re°ection e®ect in close binary systems and (b) stellar winds in O and B type
stars are discussed with their results. |
|
dc.format.extent |
48547878 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
Astronomical Observatory, Volgina 7, 11160 Beograd, Serbia. |
en |
dc.relation.uri |
http://publications.aob.rs/86/pdf/059-066.pdf |
|
dc.rights |
© Astronomical Observatory, Volgina 7, 11160 Beograd, Serbia. |
|
dc.title |
Discrete Space Theory of Radiative Transfer: Applications |
en |
dc.type |
Article |
en |