Published July 12, 2006
| Version v1
Journal article
Nucleosynthesis in Core Collapse Supernovae
Creators
- 1. INAF - Osservatorio Astronomico di Roma, Via Frascati 33, 1-00040, Monteporzio Catone, Rome (Italy)
- 2. INAF - Istituto di Astrofisica Spaziale e Fisica Cosmica, Via Fosso del Cavaliere, I-00133, Rome (Italy)
Description
We present the basic properties of the yields of our latest set of presupernova evolution and explosive nucleosynthesis of massive stars in the range between 11 and 120 M· having solar and zero metallicity
Additional details
Identifiers
- DOI
- 10.1063/1.2234389;
- arXiv
- arXiv:astro-ph/0601198v1;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 847
- Journal Issue
- 1
- Journal Page Range
- p. 99-104
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- New horizon of nuclear astrophysics and cosmology
- Acronym
- International symposium on origin of matter and evolution of galaxies 2005
- Dates
- 8-11 Nov 2005
- Place
- Tokyo (Japan)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 38045190
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ASTROPHYSICS; COSMOLOGY; NUCLEAR REACTION YIELD; NUCLEOSYNTHESIS; STAR EVOLUTION; SUPERNOVAE
- Descriptors DEC
- BINARY STARS; ERUPTIVE VARIABLE STARS; EVOLUTION; PHYSICS; STARS; SYNTHESIS; VARIABLE STARS; YIELDS
Optional Information
- Notes
- (c) 2006 American Institute of Physics