morse¶
γ Doradus (γ Dor) and slowly-pulsating B-type (SPB) stars are main-sequence stars that pulsate in low-frequency gravito-inertial modes. The morse package is dedicated to the seismic analysis of these two classes of pulsating stars. It allows you to:
find gravity-mode period spacing patterns,
perform mode identification,
measure the mean internal rotation rate,
measure the buoyancy radius of the resonant cavity,
using the list of frequencies extracted from the oscillation spectrum.