About: The flare model for X-ray variability of NGC 4258     Goto   Sponge   NotDistinct   Permalink

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Description
  • We study the variability mechanism of active galactic nuclei (AGN) within the framework of the flare model. To this end we examine the case of Seyfert/LINER galaxy NGC 4258, which is observed at high inclination angle and exhibits rapid fluctuations of the X-ray light curve. We construct a model light curve based on the assumption of magnetic flares localized in the equatorial plane. We calculate the level of variability as a function of the inclination. Highly inclined sources such as this one are particularly suitable to test the flare model because the effects of orbital motion, Doppler boosting and light bending are all expected to have maximum when the accretion disk is seen almost edge-on. The model is consistent with the NGC 4258 variability, where the obscuring material is thought to be localized mainly towards the equatorial plane.
  • We study the variability mechanism of active galactic nuclei (AGN) within the framework of the flare model. To this end we examine the case of Seyfert/LINER galaxy NGC 4258, which is observed at high inclination angle and exhibits rapid fluctuations of the X-ray light curve. We construct a model light curve based on the assumption of magnetic flares localized in the equatorial plane. We calculate the level of variability as a function of the inclination. Highly inclined sources such as this one are particularly suitable to test the flare model because the effects of orbital motion, Doppler boosting and light bending are all expected to have maximum when the accretion disk is seen almost edge-on. The model is consistent with the NGC 4258 variability, where the obscuring material is thought to be localized mainly towards the equatorial plane. (en)
Title
  • The flare model for X-ray variability of NGC 4258
  • The flare model for X-ray variability of NGC 4258 (en)
skos:prefLabel
  • The flare model for X-ray variability of NGC 4258
  • The flare model for X-ray variability of NGC 4258 (en)
skos:notation
  • RIV/67985815:_____/11:00359783!RIV12-AV0-67985815
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(GA202/09/0772), P(GA205/07/0052), P(GP205/09/P468), P(ME09036), Z(AV0Z10030501)
http://linked.open...iv/cisloPeriodika
  • June
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
http://linked.open.../riv/druhVysledku
http://linked.open...iv/duvernostUdaju
http://linked.open...titaPredkladatele
http://linked.open...dnocenehoVysledku
  • 199911
http://linked.open...ai/riv/idVysledku
  • RIV/67985815:_____/11:00359783
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • accretion disks; active galaxies; X-rays (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • FR - Francouzská republika
http://linked.open...ontrolniKodProRIV
  • [29985776B296]
http://linked.open...i/riv/nazevZdroje
  • Astronomy and Astrophysics
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...vavai/riv/projekt
http://linked.open...UplatneniVysledku
http://linked.open...v/svazekPeriodika
  • 530
http://linked.open...iv/tvurceVysledku
  • Dovčiak, Michal
  • Karas, Vladimír
  • Czerny, B.
  • Goosmann, R. W.
  • Nikolajuk, M.
  • Pecháček, Tomáš
  • Trzesniewski, T.
http://linked.open...ain/vavai/riv/wos
  • 000291027400136
http://linked.open...n/vavai/riv/zamer
issn
  • 0004-6361
number of pages
http://bibframe.org/vocab/doi
  • 10.1051/0004-6361/201016369
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