7-9 December 2016
Cochem (Mosel), Germany
Europe/Berlin timezone
Registration Nov 14th | Early bird payment Nov 30th

Aperiodic x-ray variability in Blackhole binaries

Not scheduled
Cochem (Mosel), Germany

Cochem (Mosel), Germany

Kapuzinerkloster, Klosterberg 5, 56812 Cochem
Poster HAP Workshop


Mr. armin vahdat motlagh (Istanbul Technical University)


To be able to fully describe the emission properties of a black hole binary system multi-wavelength observations are required as the inner parts of the accretion disk and the corona emit X- and Gamma- rays, outer parts of the accretion disk and the companion star emit optical and infrared emission and jets emit radiation from radio all the way to soft X-rays. In this matter i will model the x-ray variability of this systems with a new developed model PROPFLUC and compare it with previous models such as Lorentzian. Then i will utilize evolution of the outer and inner disk radius for different phases and finally i will compare the evolution in standards and outliers in the radio/X-ray correlation.

Primary author

Mr. armin vahdat motlagh (Istanbul Technical University)


Dr. Emrah Kalemci (Sabanci university)

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