A possible presence of He H+  in white dwarfs

dc.contributor.author	Gaur, V. P.
dc.contributor.author	Joshi, G. C.
dc.contributor.author	Pande, M. C.
dc.date.accessioned	2010-01-14T07:25:23Z
dc.date.available	2010-01-14T07:25:23Z
dc.date.issued	1992
dc.identifier.uri	http://hdl.handle.net/123456789/428
dc.description.abstract	In equivalent width calculations for the fundamental vibration rotation band lines of He H+ have been carried out for a non-DA white dwarf model with an effective temperature of 12000 k. Both P and R branch line with rotational quantum numbers J=3 to18 were included in the calculations. A search for these lines in helium rich white dwarfs is suggested.	en_US
dc.language.iso	en	en_US
dc.relation.ispartofseries	ass197-57
dc.subject	Astrophysics, White Dwarfs	en_US
dc.title	A possible presence of He H+ in white dwarfs	en_US
dc.type	Article	en_US