Effects of partial frequency redistribution functions R(II), R(III) and R(V) on source functions

dc.contributor.author	Mohan Rao, D
dc.contributor.author	Rangarajan, K. E
dc.contributor.author	Peraiah, A
dc.date.accessioned	2008-09-23T10:00:47Z
dc.date.available	2008-09-23T10:00:47Z
dc.date.issued	1984-06
dc.identifier.citation	Journal of Astrophysics and Astronomy, Vol. 5, No. 2, pp. 169 - 180	en
dc.identifier.issn	0250-6335
dc.identifier.uri	http://hdl.handle.net/2248/3804
dc.description.abstract	The effects of partial frequency redistribution on the formation of spectral lines have been studied. The angle-averaged R(II), R(III) and R(V) types of redistribution with isotropic phase function have been considered. Transfer equation with plane-parallel geometry is solved in isothermal atmospheres. For an atmosphere with constant thermal sources, the frequency-dependent source function S/L/(R/V/) lies below S/L/(R/III/) but above S/L/(R/II/) in the line wings.	en
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences	en
dc.relation.uri	http://ads.ari.uni-heidelberg.de/abs/1984JApA....5..169M	en
dc.subject	Atmospheric Models	en
dc.subject	Frequency Distribution	en
dc.subject	Line Spectra	en
dc.subject	Radiative Transfer	en
dc.subject	Stellar Atmospheres	en
dc.title	Effects of partial frequency redistribution functions R(II), R(III) and R(V) on source functions	en
dc.type	Article	en