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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1410
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dc.contributor.authorPeraiah, A-
dc.date.accessioned2007-03-14T06:08:30Z-
dc.date.available2007-03-14T06:08:30Z-
dc.date.issued1990-
dc.identifier.citationBASI, Vol. 18, pp. 149-165en
dc.identifier.urihttp://hdl.handle.net/2248/1410-
dc.description.abstractVarious factors influencing the formation of spectral lines are described, emphasizing the physics of stellar atmospheres. Broadening mechanisms, photon or partial frequency redistribution, the role of chemical species are briefly addressed. Emphasis is given to a discussion of geometrical and dynamical aspects, including plane parallel and spherical symmetry, the rest and the comoving frames, and aberration and advectionen
dc.format.extent350485 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectFluid dynamicsen
dc.subjectRadiative transferen
dc.titleRadiation trensfer in fast moving fluidsen
dc.typeArticleen
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