Speaker
Mr
armin vahdat motlagh
(Istanbul Technical University)
Description
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)
Co-author
Dr
Emrah Kalemci
(Sabanci university)
