Radiation trensfer in fast moving fluids

dc.contributor.author	Peraiah, A
dc.date.accessioned	2007-03-14T06:08:30Z
dc.date.available	2007-03-14T06:08:30Z
dc.date.issued	1990
dc.identifier.citation	BASI, Vol. 18, pp. 149-165	en
dc.identifier.uri	http://hdl.handle.net/2248/1410
dc.description.abstract	Various 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 advection	en
dc.format.extent	350485 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Fluid dynamics	en
dc.subject	Radiative transfer	en
dc.title	Radiation trensfer in fast moving fluids	en
dc.type	Article	en