On the evolution of stars that form electron-degenerate cores processed by carbon burning. II. Isotope abundances and thermal pulses in a 10 M⊙ model with an ONe core and applications to long-period variables, classical novae, and accretion-induced collapse

Astrophysical Journal

Volumn 460, Issue 1 PART I, 1996, Pages 489-505

  Ritossa, Claudio ^a,c   Gargía Berro, Enrique ^b   Iben Jr , Icko ^c  

^a UNIVERSITY OF BOLOGNA   (Italy)

^b UNIVERSITAT POLITÈCNICA DE CATALUNYA   (Spain)

^c UNIVERSITY OF ILLINOIS AT URBANA CHAMPAIGN   (United States)

Author keywords

Novae, cataclysmic variables; Nuclear reactions, nucleosynthesis, abundances; Stars: Abundances; Stars: AGB and post AGB; Stars: Evolution; Stars: Interiors; Stars: Variables: Long period variables

Indexed keywords

EID: 21344474270     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/176987     Document Type: Article

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