Polarization line radiative transfer in the atmospheres of magnetic white dwarfs

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3747

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DC Field	Value	Language
dc.contributor.author	Nagendra, K. N	-
dc.date.accessioned	2008-09-20T11:48:06Z	-
dc.date.available	2008-09-20T11:48:06Z	-
dc.date.issued	1987	-
dc.identifier.citation	Astronomische Nachrichten , Vol. 308, No. 5, pp. 303 - 312	en
dc.identifier.issn	0004-6337	-
dc.identifier.uri	http://hdl.handle.net/2248/3747	-
dc.description.abstract	Some physical mechanisms which can affect the Zeeman line profiles of magnetic white dwarfs are studied. The pure absorption polarization transfer equation is solved including these mechanisms. The broadening of lines in magnetic white dwarfs is briefly discussed.	en
dc.language.iso	en	en
dc.publisher	Akademie verlag GmbH	en
dc.relation.uri	http://ads.ari.uni-heidelberg.de/abs/1987AN....308..303N	en
dc.subject	Magnetic stars	en
dc.subject	Polarization characteristics	en
dc.subject	Radiative transfer	en
dc.subject	Spectral line width	en
dc.subject	Stellar atmospheres	en
dc.subject	White dwarf stars	en
dc.subject	Stellar physics	en
dc.subject	Zeeman effect	en
dc.title	Polarization line radiative transfer in the atmospheres of magnetic white dwarfs	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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