Kuldeep Singh, Indranil Chattopadhyay
Published 2018-02-16Version 1
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.
Comments: 8 pages, 6 figures, published in a special issue of JApA
Multiple X-ray bursts and the model of a spreading layer of accreting matter over the neutron star surface
Single X-ray Bursts and the Model of a Spreading Layer of Accreting Matter over the Neutron Star Surface
X-ray emissions from magnetic polar regions of neutron stars
![QR code for arXiv:1802.05850 [astro-ph.HE]](http://oss.arxitics.com/images/favicon.svg)