# Stability Analysis of Strange-Modes in Hot Massive Stars with Time-Dependent Convection

@article{Sonoi2014StabilityAO,
title={Stability Analysis of Strange-Modes in Hot Massive Stars with Time-Dependent Convection},
author={Takafumi Sonoi and Hiromoto Shibahashi},
journal={arXiv: Solar and Stellar Astrophysics},
year={2014}
}
• Published 21 April 2014
• Physics
• arXiv: Solar and Stellar Astrophysics
We carry out a nonadiabatic analysis of strange-modes in hot massive stars with time-dependent convection (TDC). In envelopes of such stars, convective luminosity is not so dominant as that in envelopes of stars in the redder side of the classical instability strip. Around the Fe opacity bump, however, convection non-negligibly contributes to energy transfer. Indeed, instability of modes excited at the Fe bump is likely to be suppressed with TDC compared with the case of adopting the frozen-in…
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