Parameter space study of magnetohydrodynamic flows around magnetized compact objects

Details Parameter space study of magnetohydrodynamic flows around magnetized compact objects Parameter space study of magnetohydrodynamic flows around magnetized compact objects

2007-06-20

arxiv.org/abs/0706.2896v1

Astronomy and Astrophysics

Astrophysics

3 pages; 4 figures; prepared on the basis of the talk presented in the MG11 Meeting on General Relativity, Berlin, July 23-29,

Scientific paper

10.1111/j.1365-2966.2006.11185.x

We solve the magnetohydrodynamic (MHD) equations governing axisymmetric flows
around neutron stars and black holes and found all possible solution topologies
for adiabatic accretion. We divide the parameter space spanned by the conserved
energy and angular momentum of the flow in terms of the flow topologies. We
also study the possibility of the formation of the MHD shock waves.

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