Single Rotating Stars and the Formation of Bipolar Planetary Nebula
We have computed new stellar evolution models that include the effects of rotation and magnetic torques under different hypotheses. The goal is to test whether a single star can sustain the rotational velocities needed in the envelope for magnetohydrodynamical(MHD) simulations to shape bipolar planetary nebulae (PNe) when high mass-loss rates take
García-Segura, G. et al.
Fecha de publicación:
3
2014