Non-thermal electromagnetic radiation from pulsating and collapsing magnetized white dwarfs

Details Non-thermal electromagnetic radiation from pulsating and collapsing magnetized white dwarfs Non-thermal electromagnetic radiation from pulsating and collapsing magnetized white dwarfs

Jun 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009jphcs.172a2051k&link_type=abstract

Journal of Physics: Conference Series, Volume 172, Issue 1, pp. 012051 (2009).

Physics

Scientific paper

The non-thermal electromagnetic radiation from pulsating and collapsing magnetized white dwarfs is considered. This radiation generates when the star magnetosphere compresses during collapse and its magnetic field greatly increases. The electric field produced involves acceleration of charged particles, which generates radiation when moving in the magnetic field. Thus the pulsating and collapsing magnetized white dwarfs can be powerful sources of electromagnetic pulses. These pulses can be observed by means of modern instruments (radio, X- and gamma- telescopes).

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