Theory of Accretion onto Neutron Stars

Details Theory of Accretion onto Neutron Stars Theory of Accretion onto Neutron Stars

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ap.....47..513a&link_type=abstract

Astrophysics (English translation of Astrofizika), v. 47, Issue 4, p. 513-518 (2004).

Astronomy and Astrophysics

Astrophysics

Stars, Neutron, Accretion, Stars - Neutron - Accretion

Scientific paper

Hydrodynamically stationary, spherically symmetric accretion onto a neutron star is examined taking the reverse effect of radiation into account. It is assumed that the plasma flow is adiabatic and that radiation is generated in a thin surface layer of the neutron star, where incoming particles are slowed down. It is shown that for stationary accretion, neither a stop, nor a substantial slowing down of the accretion flux is possible for any physically allowed conditions far from the neutron star.

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