The early mass loss history of the classical nova V1974 Cyg 1992
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Publication date
2008
Authors
Cassatella, A.
Lamers, H.J.G.L.M.
Editors
de Koter, A.
Smith, L.J.
Waters, L.B.F.M.
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Abstract
The wind of the classical nova V1974 Cygni is studied by modeling the observed profiles of the most prominent ultraviolet doublets Mg II, C II, Al III, Si IV and CIV through the Sobolev Exact Integration (SEI) method by Lamers et al. (1997). Examples are shown for the Mg ii 2800 Å doublet.
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Cassatella, A & Lamers, H J G L M 2008, The early mass loss history of the classical nova V1974 Cyg 1992. in A de Koter, L J Smith & L B F M Waters (eds), Mass loss from stars and the evolution of stellar clusters : proceedings of a workshop held at Lunteren, The Netherlands 29 May - 1 June 2006. Astronomical Society of the Pacific conference series, no. 388, Astronomical Society of the Pacific, San Francisco, pp. 153-154.