Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/75
Title: Early Nebular Stage of Nova Cygni, 1975
Authors: Prabhu, T. P
Keywords: Nova Cygni 1975;Nebular Stage;Spectroscopy;Envelope Model
Issue Date: 1977
Publisher: Indian Institue of Astrophysics, Bangalore
Citation: Kodaikanal Observatory Bulletins Series A, Vol. 2, pp. 75-84
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.
URI: http://hdl.handle.net/2248/75
ISSN: 0374-3632
Appears in Collections:Kodaikanal Observatory Bulletins (1905 - 1997 )
IIAP Publications

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