Polarization of resonance lines formed in extended spherical atmospheres

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/84

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DC Field	Value	Language
dc.contributor.author	Nagendra, K. N	-
dc.date.accessioned	2004-12-09T04:05:32Z	-
dc.date.available	2004-12-09T04:05:32Z	-
dc.date.issued	1989-04	-
dc.identifier.citation	Astrophysics and Space Science, vol. 154, no. 1, pp. 119-142	en
dc.identifier.uri	http://hdl.handle.net/2248/84	-
dc.description.abstract	The present consideration of the polarization problem posed by resonance lines in extended spherical atmospheres assumes that the atmosphere in question is at rest and emphasizes the determination of constraints that can be placed on model parameters for observations of polarization across resonance lines. A comparison is conducted of polarized lines formed under three kinds of line-scattering, namely those which are coherent, completely redistributing, and partial-frequency redistributing. Polarization's dependence on opacity laws, extendedness, and optical depth is treated in detail, as is the distribution of line intensity and polarization across the visible disk of an extended model stellar atmosphere	en
dc.format.extent	17614656 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Kluwer Academic Publishers	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1989Ap%26SS.154..119N	en
dc.subject	Stellar atmosphere	en
dc.subject	Stellar spectra	en
dc.title	Polarization of resonance lines formed in extended spherical atmospheres	en
dc.type	Article	en
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