2 papers
astro-ph2003
Instabilities of captured shocks in the envelopes of massive stars
M. Grott, W. Glatzel, S. Chernigovski
The evolution of strange mode instabilities into the non linear regime has been followed by numerical simulation for an envelope model of a massive star having solar chemical compo…
astro-ph2003
Simulation of stellar instabilities with vastly different timescales using domain decomposition
M. Grott, S. Chernigovski, W. Glatzel
Strange mode instabilities in the envelopes of massive stars lead to shock waves, which can oscillate on a much shorter timescale than that associated with the primary instability.…