Compton Broadening Due To Electron Scattering

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/230

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DC Field	Value	Language
dc.contributor.author	Peraiah, A	-
dc.contributor.author	Srinivasa Rao, M	-
dc.date.accessioned	2005-01-15T06:07:20Z	-
dc.date.available	2005-01-15T06:07:20Z	-
dc.date.issued	1993	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 12, pp. 93-100	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/230	-
dc.description.abstract	We have investigated the effects of Compton broadening due to electron scattering in the hot stellar atmosphere, quasars, AGN's etc. We considered a purely electron scattering media. The Compton effect scattering function produces the redshift and asymmetry in the line. These two effects increase as the optical depth increases. For an optical depth of 100, the emergent specific intensities become completely asymmetric in a given direction.	en
dc.format.extent	419245 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Compton broadening-Electron Scattering	en
dc.title	Compton Broadening Due To Electron Scattering	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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