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タイトルPhotoionisation modelling of Nova LMC 1990 #1
著者(英)Shore, S.; Sonneborn, G.; Sutherland, R.; Meatheringham, S. J.; Williams, R. E.; Dopita, M. A.; Starrfield, S.
著者所属(英)NASA Goddard Space Flight Center
発行日1992-01-01
1992
言語eng
内容記述Nova LMC 1990A was a very fast Ne-O-Mg nova, for which a particularly dense coverage of spectral observation in both the UV and optical was obtained. The data for the nebular phase were subjected to an analysis by the photoionization modeling code MAPPINGS 2. The following parameters were obtained: L(sub max) = 8 x 10(exp 4) solar luminosity, T(sub eff) = 2 x 10(exp 5) K and the mass of ejecta = 5/5 x 10(exp -5) solar mass. The abundnace ratios in the ejecta were similar to those obtained by Williams et al. (1985) in the case of V693 CrA 1981. The N/O ratio and the overabundance of Al is consistent with ourburst on a ONeMg white dwarf of mass approximately equal to 1.2 solar mass, but the super-Eddington luminosity, and amount of mass ejected presents some problems to theory.
NASA分類ASTROPHYSICS
レポートNO95A88830
権利Copyright


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