Published 1980
| Version v1
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Hydrodynamic studies of the nova outburst
Description
Hydrostatic studies have shown that a thermonuclear runaway will occur in the hydrogen-rich material accumulated on the surface of a degenerate star. Results of earlier studies are used to obtain models for calculations which show that the resulting thermonuclear runaway produces a nova outburst; the characteristics of this outburst depending on the carbon-oxygen abundance in the envelope
Availability note (English)
MF available from INIS under the Report Number; Available from NTIS., PC A02/MF A01.
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Additional details
Publishing Information
- Imprint Pagination
- 6 p.
- Report number
- LA-UR--80-2898
Conference
- Title
- International astronomical union colloquium 58 on stellar hydrodynamics.
- Dates
- Aug 1980.
- Place
- Los Alamos, NM, USA.
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 12583143
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- CHEMICAL COMPOSITION; HYDRODYNAMIC MODEL; NOVAE; STAR MODELS; THERMONUCLEAR REACTIONS
- Descriptors DEC
- ERUPTIVE VARIABLE STARS; MATHEMATICAL MODELS; NUCLEAR REACTIONS; NUCLEOSYNTHESIS; PARTICLE MODELS; STARS; STATISTICAL MODELS; THERMODYNAMIC MODEL; VARIABLE STARS
Optional Information
- Secondary number(s)
- CONF-800872--6.