The early mass loss history of the classical nova V1974 Cyg 1992

A. Cassatella, H.J.G.L.M. Lamers

Research output: Chapter in Book/Report/Conference proceedingChapterAcademic

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.
Original languageUndefined/Unknown
Title of host publicationMass loss from stars and the evolution of stellar clusters : proceedings of a workshop held at Lunteren, The Netherlands 29 May - 1 June 2006
EditorsA. de Koter, L.J. Smith, L.B.F.M. Waters
Place of PublicationSan Francisco
PublisherAstronomical Society of the Pacific
Pages153-154
Number of pages471
ISBN (Print)978-1-58381-644-8
Publication statusPublished - 2008

Publication series

NameAstronomical Society of the Pacific conference series
Number388

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