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Studies of neutron stars at optical/IR wavelengths

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Isolated Neutron Stars: From the Surface to the Interior

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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Correspondence to R. P. Mignani .

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Silvia Zane Roberto Turolla Dany Page

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Mignani, R.P. et al. (2007). Studies of neutron stars at optical/IR wavelengths. In: Zane, S., Turolla, R., Page, D. (eds) Isolated Neutron Stars: From the Surface to the Interior. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-5998-8_27

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