The properties of the peculiar type la supernova 1991bg - II. The amount of56Ni and the total ejecta mass determined from spectrum synthesis and energetics considerations

Monthly Notices of the Royal Astronomical Society

Volumn 284, Issue 1, 1997, Pages 151-171

  Mazzali, P A ^a   Chugai, N ^b   Turatto, M ^c   Lucy, L B ^d   Danziger, I J ^a,e   Cappellaro, E ^c   Della Valle, M ^f   Benetti, S ^e  

^a INAF OSSERVATORIO ASTRONOMICO DI TRIESTE   (Italy)

^b INSTITUTE OF ASTRONOMY   (Russian Federation)

^c INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

^d Space Telescope Europ Coord F ^*  (Germany)

^e EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^f UNIVERSITY OF PADOVA   (Italy)

Author keywords

Line: formation; Line: identification; Nuclear reactions, nucleosynthesis, abundances; Stars: abundances; Supernovae: individual: SN 1991bg

Indexed keywords

COBALT; COBALT COMPOUNDS; DECOMPOSITION; NICKEL; NUCLEAR REACTIONS; OXYGEN; SUPERNOVAE; TITANIUM COMPOUNDS; WHITE DWARFS;

LIGHT CURVES; LINE FORMATIONS; LINE:IDENTIFICATION; LOW-VELOCITY; NUCLEAR REACTIONS NUCLEOSYNTHESIS ABUNDANCES; PROPERTY; SPECTRUM SYNTHESIS; STARS ABUNDANCES; SUPERNOVA: INDIVIDUAL: SUPERNOVA 1991BG; SUPERNOVAE: INDIVIDUAL: SN 1987A;

TEMPERATURE;

EID: 4243731912     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/284.1.151     Document Type: Article

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