Published July 15, 1981
| Version v1
Journal article
Violent phase of the core helium flash
Description
The calculations described previously by Cole and Deupree were continued until the core helium flash reached a violent phase. Suitable alterations were made to the input physics, and the violent phase followed for about 5 seconds. We find a deflagration wave, not a detonation wave as previous investigators of violent core flashes have found. We attribute this difference primarily to the nonspherical nature of the burning in our two-dimensional code. Velocities of core material reach 2000 km s-1, well below either the sound speed or the escape speed. It is highly likely that some mass loss will occur, but complete disruption of the star does not occur
Additional details
Publishing Information
- Journal Title
- Astrophys. J.
- Journal Volume
- 247
- Journal Issue
- 2
- Series
- Astrophys. J.
- Journal Page Range
- 607-613
- ISSN
- 0004-637X
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 13666990
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CONVECTION; HELIUM BURNING; NUCLEOSYNTHESIS; NUMERICAL SOLUTION; STAR MODELS
- Descriptors DEC
- ENERGY TRANSFER; HEAT TRANSFER; MATHEMATICAL MODELS; STAR BURNING