The Early Mass Loss History of the Classical Nova V1974 Cyg 1992

Details The Early Mass Loss History of the Classical Nova V1974 Cyg 1992 The Early Mass Loss History of the Classical Nova V1974 Cyg 1992

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..388..153c&link_type=abstract

Mass Loss from Stars and the Evolution of Stellar Clusters ASP Conference Series, Vol. 388, proceedings of the conference held 2

Astronomy and Astrophysics

Astronomy

Scientific paper

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 C IV 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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