Published 2003
| Version v1
Journal article
Element synthesis in Novae
- 1. The University of North Carolina at Chapel Hill, Chapel Hill, North Carolina 27599-3255 (United States)
- 2. Departament de Fisica i Enginyeria Nuclear (UPC), Avinguda Victor Balaguer, s/n, E-08800 Vilanova i la Geltru, Barcelona (Spain)
- 3. Department of Physics and Astronomy, Arizona State University, Tempe, Arizona 85287-1504 (United States)
- 4. Scientific Computing, Computational Mathematics Program, Stanford University, Stanford, California 94305 (United States)
Description
Novae are fascinating astronomical objects. They occur in a binary star system consisting of a white dwarf and a companion star. During the evolution of the binary star system, matter is transferred onto the white dwarf surface and a thermonuclear runaway occurs. As a result, the material that is ejected into interstellar space represents an observational signature of the underlying white dwarf, the accreted matter before the outburst, and the complicated explosion itself. In the present work, we will review some of the recent advances in our understanding of the nuclear physics input for this complex phenomenon. (Author)
Additional details
Publishing Information
- Journal Title
- Revista Mexicana de Fisica
- Journal Volume
- 49
- Journal Issue
- Suppl.4
- Journal Page Range
- p. 45-49
- ISSN
- 0035-001X
- CODEN
- RMXFAT
Conference
- Title
- 26. Symposium on Nuclear Physics
- Dates
- 6-9 Jan 2003
- Place
- Taxco, Guerrero (Mexico)
INIS
- Country of Publication
- Mexico
- Country of Input or Organization
- Mexico
- INIS RN
- 35021073
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- DIAGRAMS; KEV RANGE; MAGNESIUM 24; MASS NUMBER; NOVAE; NUCLEOSYNTHESIS; REACTION KINETICS; SODIUM 23; THERMONUCLEAR REACTIONS; WHITE DWARF STARS
- Descriptors DEC
- ALKALINE EARTH ISOTOPES; BINARY STARS; DWARF STARS; ENERGY RANGE; ERUPTIVE VARIABLE STARS; EVEN-EVEN NUCLEI; INFORMATION; ISOTOPES; KINETICS; LIGHT NUCLEI; MAGNESIUM ISOTOPES; NUCLEAR REACTIONS; NUCLEI; NUCLEOSYNTHESIS; ODD-EVEN NUCLEI; SODIUM ISOTOPES; STABLE ISOTOPES; STARS; SYNTHESIS; VARIABLE STARS