Evolutionary sequences for Nova V1974 Cygni using new nuclear reaction rates and opacities

Monthly Notices of the Royal Astronomical Society

Volumn 296, Issue 3, 1998, Pages 502-522

  Starrfield, S ^a   Truran, J W ^b   Wiescher, M C ^c   Sparks, W M ^d  

^a ARIZONA STATE UNIVERSITY   (United States)

^b UNIVERSITY OF CHICAGO   (United States)

^c UNIVERSITY OF NOTRE DAME   (United States)

^d LOS ALAMOS NATIONAL LABORATORY   (United States)

Author keywords

Convection; Novae, cataclysmic variables; Nuclear reactions, nucleosynthesis, abundances; Stars: activity; Stars: individual: Nova V1974 Cygni; White dwarfs

Indexed keywords

BUDGET CONTROL; GIANT STARS; MAGNESIUM; NEON; NUCLEOSYNTHESIS; OXYGEN; REACTION INTERMEDIATES; REACTION RATES;

CONVECTION; NOVAE CATACLYSMIC VARIABLES; NUCLEAR REACTION RATES; NUCLEAR REACTIONS NUCLEOSYNTHESIS ABUNDANCES; REACTION NETWORK; REACTIONS RATES; STAR: ACTIVITY; STAR: INDIVIDUAL: NOVA V1974 CYGNI; STARS: INDIVIDUAL: PROXIMA CENTAURI; TOTAL ENERGY;

WHITE DWARFS;

EID: 0001544514     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01312.x     Document Type: Article

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