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1997ApJ...475..803C - Astrophys. J., 475, 803-811 (1997/February-1)
The shell of recurrent nova T Pyxidis: a model based on shocks.
CONTINI M. and PRIALNIK D.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): Stars: Novae, Cataclysmic Variables - Stars: Individual Constellation Name: T Pyxidis - Shock Waves - Stars: Abundances - Stars: Mass Loss - Stars: White Dwarfs
Simbad objects: 7
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