HIGHLIGHTS
- who: u03b2 Pictoris et al. from the University of Cambridge, United Kingdom have published the paper: 2D modelling of pulsating stars with rapid rotation, in the Journal: (JOURNAL)
- what: The effects of centrifugal acceleration on the hydrostatic equilibrium of the model are crucial for calculating pulsations, even when the adiabatic approximation is being made, i.e., where energy exchanges are neglected during the pulsations. Some of the important goals in studying such oscillations include determining the stability of neutron This approach has the advantage of using models in which the energy equation is satisfied in . . .
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