Violet absorption edges of C IV lines in Wolf-Rayet spectra: possible superposition with diffuse interstellar bands at 5780 Å and 5797 Å

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5034

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DC Field	Value	Language
dc.contributor.author	Giridhar, S	-
dc.contributor.author	Bappu, M. K. V	-
dc.date.accessioned	2010-02-24T11:06:58Z	-
dc.date.available	2010-02-24T11:06:58Z	-
dc.date.issued	1978	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 2, pp. 161–163	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/5034	-
dc.description.abstract	It is shown that the violet edges normally seen in Wolf-Rayet stars around 5800Å are principally due to displaced C IV absorption. The diffuse interstellar bands are seldom of comparable strength and can be seen separately if the absorption characteristics of the envelope of the Wolf-Rayet stars are such as to avoid an overlap between the two.	en
dc.language.iso	en	en
dc.publisher	Indian Institute of Astrophysics	en
dc.rights	© Indian Institute of Astrophysics	en
dc.subject	Interstellar Bands	en
dc.subject	Spectra:Wolf-Rayet Stars	en
dc.subject	Wolf-Rayet Stars	en
dc.subject	Diffuse Interstellar Bands	en
dc.subject	Violet Absorption Edges	en
dc.title	Violet absorption edges of C IV lines in Wolf-Rayet spectra: possible superposition with diffuse interstellar bands at 5780 Å and 5797 Å	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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