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Probing the neutron star spin evolution in the young Small Magellanic Cloud Be/X‐ray binary SXP 1062Popov, S. B.; Turolla, R.
Monthly notices of the Royal Astronomical Society. Letters, March 2012, 2012-03-01, 20120301, Letnik: 421, Številka: 1Journal Article
ABSTRACT The newly discovered Be/X‐ray binary in the Small Magellanic Cloud, SXP 1062, provides the first example of a robust association with a supernova remnant (SNR). The short age estimated for the SNR qualifies SXP 1062 as the youngest known source in its class, . As such, it allows us to test current models of magnetorotational evolution of neutron stars in a still unexplored regime. Here we discuss possible evolutionary scenarios for SXP 1062 in an attempt to reconcile its long spin period, , and short age. Although several options can be considered, like an anomalously long initial period or the presence of a fossil disc, our results indicate that SXP 1062 may host a neutron star born with a large initial magnetic field, typically in excess of ∼ 1014 G, which then decayed to ∼ 1013 G.
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