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Table · dataset · 2016

Tomographic modelling of H 1743-322

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Results of fitting a tomographic model to the ~4s quasi periodic oscillation (QPO) in XMM-Newton and NuSTAR data from the black hole X-ray binary system H 1743-322.

Description

This is an animated version of Fig 3 in Ingram et al (2016). The most intensely illuminated patches of the disc rotate about the disc surface, causing the iron line to rock from red to blue shifted during a QPO cycle.

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Physical sciences
Inferred from text
Astronomical sciences 75%

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DataCite10.6084/m9.figshare.350393315 d agoJSON v1
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concepts[field].local:field:astronomymapping · DataCitevocabulary-mapper@1.0.0keywords['Astrophysics']
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