Thin disk models of anomalous X-ray pulsars

Ekşi, Kazım Yavuz and Alpar, M. Ali (2004) Thin disk models of anomalous X-ray pulsars. In: 2nd BeppoSAX Conference on Restless High-Engery Universe, Amsterdam, Netherlands

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Official URL: http://dx.doi.org/10.1016/j.nuclphysbps.2004.04.088


We discuss the options of the fall-back disk model of Anomalous X-Ray Pulsars (AXPs). We argue that the power-law index of the mass inflow rate during the propeller stage can be lower than those employed in earlier models. We take into account the effect of the super-critical mass inflow at the earliest stages on the inner radius of the disk and argue that the system starts as a propeller. Our results show that, assuming a fraction of the mass inflow is accreted onto the neutron star, the fall-back disk scenario can produce AXPs for acceptable parameters.

Item Type:Papers in Conference Proceedings
Subjects:Q Science > QC Physics
ID Code:1517
Deposited By:M. Ali Alpar
Deposited On:27 Dec 2004 02:00
Last Modified:25 May 2011 14:24

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