Optical,ultraviolet, and infrared observations of isolated neutron stars |
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Authors: | Roberto P Mignani |
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Institution: | MSSL-UCL, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, UK |
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Abstract: | Forty years passed 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 the results from recent observations. |
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Keywords: | Astrophysics Neutron stars Multi-wavelength observations |
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