Relativistic Jets from Accretion-Induced Collapsing White Dwarfs

Details Relativistic Jets from Accretion-Induced Collapsing White Dwarfs Relativistic Jets from Accretion-Induced Collapsing White Dwarfs

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..372..411k&link_type=abstract

15th European Workshop on White Dwarfs ASP Conference Series, Vol. 372, proceedings of the conference held 7-11 August, 2006 in

Astronomy and Astrophysics

Astronomy

Scientific paper

The relativistic jets in the magnetosphere of accretion-induced collapsing white dwarfs are considered. These jets will form in the polar caps of the magnetosphere, when a stellar magnetic field increases during collapse and the charged particles will accelerate. These jets will generate the non-thermal radiation. The analysis of particle dynamics and its emission in the stellar magnetosphere under collapse show that accretion-induced collapsing white dwarfs can by powerful sources of jets and non-thermal radiation.

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