Damping rates
the linewidths of individual oscillation modes were predicted to be available for a few main-sequence stars with T$_{\rm eff}$ < 5500 K.
Technical definition
The rates at which oscillation modes lose energy and become less pronounced.
the linewidths of individual oscillation modes were predicted to be available for a few main-sequence stars with T$_{\rm eff}$ < 5500 K.
The rates at which oscillation modes lose energy and become less pronounced.