On the stability of a slow deflagration front at the surface of a degenerate star

Details On the stability of a slow deflagration front at the surface of a degenerate star On the stability of a slow deflagration front at the surface of a degenerate star

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..69..217b&link_type=abstract

Astrophysics and Space Science, vol. 69, no. 1, May 1980, p. 217-225.

Computer Science

Numerical Analysis

3

Deflagration, Hydrodynamic Equations, Nuclear Reactions, Stellar Evolution, Boundary Value Problems, Numerical Analysis, Stellar Mass Ejection, Time Dependence

Scientific paper

On the surface of a degerate star, a slow nuclear combustion process
with a wake of escaping matter can exist. The evolution of this process
has been studied by solving the non- adiabatic, time-dependent
hydrodynamic equations. It has been found that this flow is almost
stationary and is stable against small spherical symmetric perturbations

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