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arXiv · 0908.1010

Multi-wavelength observations of isolated neutron stars

Roberto P. Mignani
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Abstract

Forty years elapsed since the optical identification of the first isolated neutron star (INS), the Crab pulsar. 25 INSs have been now identified in the optical (O), near-ultraviolet (nUV), or near-infrared (nIR), hereafter UVOIR, including rotation-powered pulsars (RPPs), magnetars, and X-ray-dim INSs (XDINSs), while deep investigations have been carried out for compact central objects (CCOs), Rotating RAdio transients (RRATs), and high-magnetic field radio pulsars (HBRPs). In this review I describe the status of UVOIR observations of INSs, their emission properties, and I present recent results.

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Roberto P. Mignani. 2009-08-07. Multi-wavelength observations of isolated neutron stars. https://arxiv.org/abs/0908.1010

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