Emission-line profiles from expanding envelopes

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1993

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DC Field	Value	Language
dc.contributor.author	Bappu, M. K. V	-
dc.contributor.author	Menzel, D. H	-
dc.date.accessioned	2007-11-30T12:04:40Z	-
dc.date.available	2007-11-30T12:04:40Z	-
dc.date.issued	1954-05	-
dc.identifier.citation	The Astrophysical Journal, Vo, 119, No. 3, pp. 508-518	en
dc.identifier.uri	http://hdl.handle.net/2248/1993	-
dc.description.abstract	We have developed a method for calculating the emission-line profiles from an expanding envelope. The method applies to an envelope where the emission intensity varies with latitude. Some typically illustrative cases are considered.	en
dc.format.extent	663059 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	University of Chicago Press	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1954ApJ...119..508V	en
dc.subject	Emission Bands	en
dc.subject	Emission Lines Profiles	en
dc.subject	M.K.V. Bappu	en
dc.title	Emission-line profiles from expanding envelopes	en
dc.type	Article	en
Appears in Collections:	M.K. Vainu Bappu ( 1960 - 1982 )

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