Study of Magnetized accretion flow with cooling processes
High Energy Astrophysical Phenomena
2018-03-14 v1
Abstract
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.
Cite
@article{arxiv.1802.05850,
title = {Study of Magnetized accretion flow with cooling processes},
author = {Kuldeep Singh and Indranil Chattopadhyay},
journal= {arXiv preprint arXiv:1802.05850},
year = {2018}
}
Comments
8 pages, 6 figures, published in a special issue of JApA