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SUMMARY:Broadband Emission of Magnetar Wind Nebulae
DTSTART;VALUE=DATE-TIME:20151029T063000Z
DTEND;VALUE=DATE-TIME:20151029T065000Z
DTSTAMP;VALUE=DATE-TIME:20261013T214837Z
UID:indico-contribution-974@indico.icrr.u-tokyo.ac.jp
DESCRIPTION:Speakers: Shuta Tanaka (ICRR\, The University of Tokyo)\nRotat
 ion-powered pulsars release their rotational energy as relativistic magnet
 ized plasma and create pulsar wind nebulae (PWNe) around them.\nAlthough m
 agnetars are considered as magnetically powered pulsar\, they also release
  their rotational energy by the wind.\nThis is obvious from the fact that 
 they are spinning down.\nWe have been detected PWNe around energetic pulsa
 rs which have spin-down power of more than 10^36 erg/s\, typically.\nIn th
 is study\, we consider the wind nebula around magnetars (MWN).\nAlthough t
 hey have relatively small spin-down power\, magnetars would have had a lar
 ge spin-down power at their birth because they spin down rapidly.\nHere\, 
 we construct an one-zone spectral model of MWN considering spin-down evolu
 tion of magnetar and apply to some objects which are claimed to have MWN i
 n X-rays.\n\nhttps://indico.icrr.u-tokyo.ac.jp/event/23/contributions/974/
LOCATION: Room 5.6
URL:https://indico.icrr.u-tokyo.ac.jp/event/23/contributions/974/
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