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Studies of Neutron Stars at Optical/IR Wavelengths

R. P. Mignani·S. Bagnulo·A. De Luca·G. L. Israel·G. Lo Curto·C. Motch·R. Perna·N. Rea·R. Turolla·S. Zane
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Abstract

In the last years, optical studies of Isolated Neutron Stars (INSs) have expanded from the more classical rotation-powered ones to other categories, like the Anomalous X-ray Pulsars (AXPs) and the Soft Gamma-ray Repeaters (SGRs), which make up the class of the magnetars, the radio-quiet INSs with X-ray thermal emission and, more recently, the enigmatic Compact Central Objects (CCOs) in supernova remnants. Apart from 10 rotation-powered pulsars, so far optical/IR counterparts have been found for 5 magnetars and for 4 INSs. In this work we present some of the latest observational results obtained from optical/IR observations of different types of INSs.

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R. P. Mignani, S. Bagnulo, A. De Luca, G. L. Israel, G. Lo Curto, C. Motch, R. Perna, N. Rea, R. Turolla, S. Zane. 2006-08-01. Studies of Neutron Stars at Optical/IR Wavelengths. https://doi.org/10.1007/s10509-007-9340-z

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