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Astronomical Observatory of the Jagiellonian University

Faculty of Physics, Astronomy and Applied Computer Science
Jagiellonian University, Cracow, Poland

ul. Orla 171
30-244 Kraków
POLAND
tel.: +48

12 6238 620

12 6238 629

fax.: +48

12 425 1318

A systematic study of microvariability in total flux and polarization in optical band for blazar sources

Active Galactic Nuclei (AGNs) consists of galaxies with extremely bright nucleus, so much so, that they usually outshine the light from other galaxy parts such as arms or bulges. The reason behind intense power of AGN is believed to be the super massive black hole accreting matter from its vicinity at the center of galaxy. Sometimes, such systems are known to erupt powerful, narrow beam of high velocity charged particles. If one happens to view such a systems along the line of sight of these eruptions (jets) are called blazars. The emission from blazar jets is Doppler boosted, leading to extreme luminosities and flux variability and apparent superluminal motion shown by the ejecta. Not only such systems show extreme luminosities, it also varies on all observable timescales ranging from years to minutes with amount of energy dissipated equal to a million Suns in few hours timescale.
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Komunikat Dziekana WFAIS UJ w sprawie rozprzestrzeniania się COVID-19
Komunikat Prodziekana WFAIS UJ do spraw studiów

Kraków, 2020, Jul 18th - Aug 2nd
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