Answers are grounded in this paper and cite their sources.
The non-linear pulsations of vibrationally unstable main sequence stars of between 70 and 210 M⊙ are studied using numerical methods directly. Non-linear solutions are investigated for various amplitudes for short periods of time. The results are found to be in qualitative agreement with those obtained in a previous paper using a perturbation technique. The results are found to be different from those given by other authors. In particular no mass loss is found. Possible reasons for the discrepancy are given.
No takes yet. Share an insight, caveat, or question.
Papaloizou et al. (1973) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: