RII partial frequency redistribution function and its effects on the formation of lines in expanding spherical atmospheres

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5022

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DC Field	Value	Language
dc.contributor.author	Peraiah, A	-
dc.date.accessioned	2010-02-19T12:42:56Z	-
dc.date.available	2010-02-19T12:42:56Z	-
dc.date.issued	1979-11	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 2, No. 3, pp. 203 – 212	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/5022	-
dc.description.abstract	The redistribution in frequency in lines formed in atmospheres in which the matter is moving radially outwards with velocity gradients is studied in the rest frame of the star. We velocity gradients is studied in the rest frame of the star. We have considered the RII angle averaged function (see Hummer 1962) with radiation damping in the atom’s rest frame and assumed a non LTE two level atom.	en
dc.language.iso	en	en
dc.publisher	Indian Institute of Astrophysics	en
dc.rights	© Indian Institute of Astrophysics	en
dc.subject	RII Partial Frequency Redistribution Function	en
dc.subject	Radiative Transfer in Spherical Symmetry	en
dc.subject	Expanding Atmospheres	en
dc.subject	Line Formation:Stellar Atmospheres	en
dc.subject	Radiative Transfer	en
dc.title	RII partial frequency redistribution function and its effects on the formation of lines in expanding spherical atmospheres	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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