Formation Scenario of Magnetars: The Puzzle of Isolation

dc.creatorPrasad, Nirvikar
dc.date2008-01-09
dc.date.accessioned2026-07-07T08:53:28Z
dc.date.available2026-07-07T08:53:28Z
dc.descriptionMagnetars (SGRs and AXPs) are one of the most evolutionary paths of a neutron star. These objects have an ultra-strong magnetic field $B \sim 10^{15}$ G at their surface and show persistent X-ray pulsations and transient bursts. Till date there are 14 magnetars known: 5 SGRs (4 confirmed, 1 candidate) and 9 AXPs (7 confirmed, 2 candidates). It is an open puzzle that all these objects are isolated and none have been found in binaries. We discuss the formation scenario which can lead to such a situation.
dc.descriptionPrepared for the conference "40 Years of Pulsars: Millisecond Pulsars, Magnetars, and More", August 12-17, 2007, McGill University, Montreal, Canada
dc.identifierhttps://arxiv.org/abs/0801.1365
dc.identifierhttp://arxiv.org/abs/0801.1365
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/145634
dc.subjectAstrophysics
dc.titleFormation Scenario of Magnetars: The Puzzle of Isolation
dc.typetext

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