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2006MNRAS.370L..14V - Mon. Not. R. Astron. Soc., 370, L14-L18 (2006/July-3)
Supernova remnant energetics and magnetars: no evidence in favour of millisecond proto-neutron stars.
VINK J. and KUIPER L.
Abstract (from CDS):
We therefore do not find evidence that magnetars are formed from rapidly rotating proto-neutron stars, allowing for the possibility that they descend from stellar progenitors with high magnetic field cores, and discuss the merits of both formation scenarios.
In an appendix we describe the analysis of XMM-Newton observations of Kes 73 and N49 used to derive the explosion energies for these remnants.
Abstract Copyright: 2006 The Authors. Journal compilation © 2006 RAS
Journal keyword(s): stars: magnetic fields - stars: neutron - ISM: supernova remnants - ISM: individual: N49 - ISM: individual: Kes 73 - ISM: individual: CTB 109
CDS comments: In Chap. 2: AX J1845-045 is a misprint for AX J1845.0-0258
Simbad objects: 13
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