On the mechanism of thermalization a plasma infalling onto magnetized neutron stars

Details On the mechanism of thermalization a plasma infalling onto magnetized neutron stars On the mechanism of thermalization a plasma infalling onto magnetized neutron stars

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982acns.rept..289y&link_type=abstract

In Max-Planck Inst. Phys. and Astrophys. Accreting Neutron Stars p 289-292 (SEE N83-15179 05-88)

Astronomy and Astrophysics

Astrophysics

Deceleration, Neutron Stars, Stellar Magnetic Fields, Stellar Mass Accretion, Thermal Energy, Collisional Plasmas, Conservation Equations, Cyclotron Radiation, Kinetic Energy, Mathematical Models, Momentum, Stellar Winds

Scientific paper

Preliminary results of deceleration calculations for matter infalling
onto a strongly magnetized neutron star are given. The validity of both
models of thermalization are given. It was found that for accretion
rates approximately greater than 100,000 gr.cm(-2)sec(-1), stationary,
collisionless shock solution do not exist.

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