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

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