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Study of Magnetized accretion flow with cooling processes

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arxiv 1802.05850 v1 pith:GJ5O7CAM submitted 2018-02-16 astro-ph.HE

Study of Magnetized accretion flow with cooling processes

Kuldeep Singh , Indranil Chattopadhyay This is my paper
classification astro-ph.HE
keywords accretioncoolingflowshockstarsurfacecyclotronmagnetized
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We have studied shock in magnetized accretion flow/funnel flow in case of neutron star with bremsstrahlung cooling and cyclotron cooling. All accretion solutions terminate with a shock close to the neutron star surface, but at some region of the parameter space, it also harbours a second shock away from the star surface. We have found that cyclotron cooling is necessary for correct accretion solutions which match the surface boundary conditions.

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