Rapid Spindown of SGR 1900+14 Following Its Superburst

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dc.creatorPalmer, David M.
dc.date2001-03-24
dc.date.accessioned2026-07-07T01:58:01Z
dc.date.available2026-07-07T01:58:01Z
dc.descriptionSGR 1900+14 had a brief episode of exceedingly rapid spindown immediately following its 1998 Aug. 27 superburst. On a timescale of hours, it increased its period by a part in 10^4. The corresponding Pdot ~ 10^{-8} is orders of magnitude higher than the typical quiescent rate of Pdot ~ 6x10^{-11}.
dc.descriptionSubmitted to Mem.S.A.It. for inclusion in the proceedings of 'Soft Gamma Repeaters: The Rome 2001 Mini-Workshop'. (6 pages, requires memsait.sty, included)
dc.identifierhttps://arxiv.org/abs/astro-ph/0103404
dc.identifierhttp://arxiv.org/abs/astro-ph/0103404
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2612
dc.subjectAstrophysics
dc.titleRapid Spindown of SGR 1900+14 Following Its Superburst
dc.typetext

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