Early Nebular Stage of Nova Cygni, 1975

dc.contributor.author	Prabhu, T. P
dc.date.accessioned	2004-12-01T06:17:15Z
dc.date.available	2004-12-01T06:17:15Z
dc.date.issued	1977
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 2, pp. 75-84	en
dc.identifier.issn	0374-3632
dc.identifier.uri	http://hdl.handle.net/2248/75
dc.description.abstract	The emission line profiles of the spectrum of the spectrum of the envelope of Nova V 1500 Cyg, 1975 are studied. The spectral region covers LamdaLamda 3700-8800. The velocity structure of the profiles and the time variation of both the velocities and intensities of the emission peaks of HAlpha are interpreted as due to an expanding system of rings at different latitudes with respect to a common polar axis. The envelope was optically thick to Balmer line radiation and was thinning out rapidly during the period of observations.	en
dc.format.extent	382183 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Indian Institue of Astrophysics, Bangalore	en
dc.subject	Nova Cygni 1975	en
dc.subject	Nebular Stage	en
dc.subject	Spectroscopy	en
dc.subject	Envelope Model	en
dc.title	Early Nebular Stage of Nova Cygni, 1975	en
dc.type	Article	en