Self-Similar Solutions in the Theory of Flare-Ups in Novae - Part Two

Details Self-Similar Solutions in the Theory of Flare-Ups in Novae - Part Two Self-Similar Solutions in the Theory of Flare-Ups in Novae - Part Two

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..95..105s&link_type=abstract

Astrophysics and Space Science, Volume 95, Issue 1, pp.105-109

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

The self-similar isothermal flow of a gas, moving under the
gravitational attraction of a central body of fixed mass behind a
spherical shock wave driven out by a propelling contact surface into a
non-uniform stationary atmosphere is investigated. The total energy of
the wave increases with time obeying a power-law.

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