Self-similar pulsations of gas in stars

Details Self-similar pulsations of gas in stars Self-similar pulsations of gas in stars

Oct 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978pazh....4..397b&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 4, Sept.-Oct. 1978, p. 397-401.) Soviet Astronomy Letters, vol. 4, Sept.-Oct. 1978, p.

Astronomy and Astrophysics

Astronomy

Gas Explosions, Stellar Models, Supernovae, Gas Dynamics, Shock Waves

Scientific paper

New solutions to the standard stellar explosion model are obtained,
wherein retarding radial gas oscillations develop after the shock wave
has passed. The conditions for dispersal of the entire mass of gas
comprising the star are investigated.

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