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Paper: The Early Mass Loss History of the Classical Nova V1974 Cyg 1992
Volume: 388, Mass Loss from Stars and the Evolution of Stellar Clusters
Page: 153
Authors: Cassatella, A.; Lamers, H.J.G.L.M.
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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