Polarization line radiative transfer in the atmospheres of magnetic white dwarfs

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