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On the origin of hyperfast neutron stars

Gvaramadze, VV, Gualandris, A and Zwart, SP (2007) On the origin of hyperfast neutron stars IAU Symp., 246. pp. 365-366.

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Abstract

We propose an explanation for the origin of hyperfast neutron stars (e.g. PSR B1508+55, PSR B2224+65, RX J0822-4300) based on the hypothesis that they could be the remnants of a symmetric supernova explosion of a high-velocity massive star (or its helium core) which attained its peculiar velocity (similar to that of the neutron star) in the course of a strong three- or four-body dynamical encounter in the core of a young massive star cluster. This hypothesis implies that the dense cores of star clusters (located either in the Galactic disk or near the Galactic centre) could also produce the so-called hypervelocity stars -- the ordinary stars moving with a speed of ~1000 km/s.

Item Type: Article
Authors :
NameEmailORCID
Gvaramadze, VVUNSPECIFIEDUNSPECIFIED
Gualandris, Aa.gualandris@surrey.ac.ukUNSPECIFIED
Zwart, SPUNSPECIFIEDUNSPECIFIED
Date : 27 December 2007
Identification Number : https://doi.org/10.1017/S1743921308015962
Uncontrolled Keywords : astro-ph, astro-ph
Related URLs :
Depositing User : Symplectic Elements
Date Deposited : 17 May 2017 13:00
Last Modified : 17 May 2017 15:07
URI: http://epubs.surrey.ac.uk/id/eprint/837582

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