Published 1987
| Version v1
Book
Nucleosynthesis and supernovae produced by late time neutrino heating
Description
The composition of matter injected into the interstellar medium by supernovae is determined partly by the physics of the explosion and partly by the evolutionary history of the progenitor star. This talk will discuss the role of the explosion itself in determining elemental abundances of the ejecta, focusing on core collapse supernovae (typically associated with observational Type II events). In particular, the nucleosynthesis produced by progenitor stars with mass greater than 25 solar masses and exploding by the late time neutrino heating mechanism will be discussed
Additional details
Publishing Information
- Publisher
- American Chemical Society.
- Imprint Place
- Washington, DC (USA)
- Imprint Title
- 194th national meeting of the American Chemical Society, Division of Nuclear Chemistry and Technology
- Journal Page Range
- p. 22.
Conference
- Title
- American Chemical Society Division of Nuclear Chemistry and Technology meeting.
- Dates
- 30 Aug - 4 Sep 1987.
- Place
- New Orleans, LA (USA).
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 19074562
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- COSMIC GASES; COSMOCHEMISTRY; INTERSTELLAR GRAINS; NEUTRINOS; NUCLEOSYNTHESIS; ORIGIN; STAR EVOLUTION; STARS; SUPERNOVAE
- Descriptors DEC
- BINARY STARS; CHEMISTRY; ELEMENTARY PARTICLES; ERUPTIVE VARIABLE STARS; FERMIONS; FLUIDS; GASES; LEPTONS; MASSLESS PARTICLES; PARTICLES; SYNTHESIS; VARIABLE STARS