Near‐Infrared and Ultraviolet Spectrophotometry of Symbiotic Novae
نویسندگان
چکیده
منابع مشابه
Recurrent Novae , Classical Novae , Symbiotic Novae , and Population II
Light curve analysis of decay phase of nova outburst are summarized. Nova duration is determined by the strong wind mass-loss which depends only on the white dwarf mass. Fast novae correspond very massive white dwarfs and very slow novae correspond almost lower mass limit of white dwarfs. This relation is shown in both of classical novae and recurrent novae. Light curves are theoretically repro...
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ژورنال
عنوان ژورنال: The Astrophysical Journal Supplement Series
سال: 1999
ISSN: 0067-0049,1538-4365
DOI: 10.1086/313197