English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

We present a generally applicable formalism for modeling the emission,absorption, reflection, and reprocessing of radiation by moving plasma streamsclose to a Kerr Black hole. The formalism can be used to investigate theobservational signatures of a wide range of phenomena, including: (i) thereflection of coronal X-ray radiation off plasma plunging from the inner edgeof a black hole accretion disk towards the black hole; (ii) the reflection ofcoronal X-ray emission off the upper layers of a geometrically thick accretionflow; (iii) the illumination of the accretion disk by a corona moving withrelativistic velocities towards or away from the accretion disk; (iv) theemission from a jet forming close to the black hole. After introducing thegeneral relativistic treatment, we show the results for a fast wind formingclose to a Kerr black hole. The approach presented here can be used to modelX-ray spectral, timing, reverberation, and polarization data.

Generally Applicable Formalism for Modeling the Observable Signatures of Inflows, Outflows, and Moving Coronal Plasma Close to Kerr Black Holes