Speaker
Ms
Yelyzaveta Zhyhaniuk
(Taras Shevchenko National University of Kyiv, Kyiv, Ukraine)
Description
Cygnus A is a giant elliptical galaxy, one of the most powerful radio galaxy. Like other radio galaxies, its activity is determined by active galactic nucleus (AGN) - supermassive black hole, surrounded by accretion disk, and with two relativistic jets, diverging in opposite directions from the supermassive black hole. We investigate the two hotspots - A and B - at the end of the eastern relativistic jet of Cygnus A. We analyze the X-ray emission of these hotspots using observational data from Chandra Data Archive and estimate the mechanism(s) of generation of X-ray emission.
Author
Ms
Yelyzaveta Zhyhaniuk
(Taras Shevchenko National University of Kyiv, Kyiv, Ukraine)
Co-authors
Prof.
B. I. Hnatyk
(Astronomical Observatory of Taras Shevchenko National University of Kyiv, Kyiv, Ukraine)
Dr
V. V. Marchenko
(Astronomical Observatory, Jagiellonian University, Krakow, Poland)
