dr Krzysztof Hryniewicz2020.06.15 23:20 - admin-bp4
E-mail: name.firstlastname (at) domain
My research interest include Active Galactic Nuclei and accreting sources. AGN and their brightest counterparts: quasars are the most luminous persistent sources in the universe. They are best known because of distinctive spectral features: optical-UV continuum called the Big Blue Bump, X-ray emission and broad emission lines. I am focused on accretion disc emission which is responsible for optical-UV continuum emission and its interplay with Broad/Intermediate Emission Line Regions as well as their signatures in both emission and absorption. In my work I use both observational data and theoretical models.