Studies of Neutron Stars at Optical/IR Wavelengths

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dc.creatorMignani, R. P.
dc.creatorBagnulo, S.
dc.creatorDe Luca, A.
dc.creatorIsrael, G. L.
dc.creatorCurto, G. Lo
dc.creatorMotch, C.
dc.creatorPerna, R.
dc.creatorRea, N.
dc.creatorTurolla, R.
dc.creatorZane, S.
dc.date2006-08-01
dc.date.accessioned2026-07-07T10:39:41Z
dc.date.available2026-07-07T10:39:41Z
dc.descriptionIn 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.
dc.description8 pages, 6 Postscript figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0608025
dc.identifierhttp://arxiv.org/abs/astro-ph/0608025
dc.identifierAstrophys.SpaceSci.308:203-210,2007
dc.identifierdoi:10.1007/s10509-007-9340-z
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/181117
dc.subjectAstrophysics
dc.titleStudies of Neutron Stars at Optical/IR Wavelengths
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