Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2010-11-04
Mod. Phys. Lett. A, Vol. 26, No. 5 (2011) pp. 359-366
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Mod. Phys. Lett. A 26 (2011) 359-366
Scientific paper
We study radiative activity of magnetic white dwarf undergoing torsional vibrations about axis of its own dipole magnetic moment under the action of Lorentz restoring force. It is shown that pulsating white dwarf can convert its vibration energy into the energy of magneto-dipole emission, oscillating with the frequency equal to the frequency of Alfv\'en torsional vibrations, provided that internal magnetic field is decayed. The most conspicuous feature of the vibration energy powered radiation in question is the lengthening of periods of oscillating emission; the rate of period elongation is determined by the rate magnetic field decay.
Bastrukov S. I.
Molodtsova I. V.
Xu Ren Xin
Yu Jeffrey W.
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