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Initial parameters of neutron stars

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arxiv 1206.2819 v1 pith:MILN4SV2 submitted 2012-06-13 astro-ph.HE

S.B. Popov (Sternberg Astronomical Institute) , R. Turolla (University of Padova , Mullard Space Science Lab. UCL) This is my paper · ORCID
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keywords low-fieldobjectsbirthccoscompactneutronratestars
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abstract

A subpopulation of neutron stars (NSs), known as central compact objects (CCOs) in supernova remnants, are suspected to be low-field objects basing on $P$-$\dot P$ measurements for three of them. The birth rate of low-field NSs is probably comparable with the birth rate of normal radio pulsars. However, among compact objects in High-Mass X-ray Binaries (HMXBs) we do not see robust candidates for low-field NSs. We propose that this contradiction can be solved if magnetic fields of CCOs was buried due to strong fall-back, and then the field emerges on the time scale $10^4$-$10^5$ yrs.

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