In conventional theoretical asteroseismic investigations, the normal choice always lies in the application of plane-wave analysis despite the inherent geometrical curvature effects of the emitting spherical stellar source. May I, therefore, get some helpful study materials dealing lucidly with radial and non-radial oscillations of magnetized spherical stars?
Dear Karmakar,
It is very difficult (if not impossible) to get a material which could shows the magnetism of one star. The answer is because the plasma of one star is at a very high temperature and within a fast-rotation star. Some new pulsars can reach a huge magnetic field, 10^8 T which are impossible to get here in Earth.
Dear Dr. Daniel,
Thanks a lot for response.
Further developments with asteroseismic descriptions are welcome.
Kind regards,
PK Karmakar
Physics, Tezpur University
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