activity
19972026
most citedThe origin of the Broad Line Region in Active Galactic Nuclei

271 citations · 4.6k across the 192 of their papers we have counts for

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Showing 2019 · astro-ph.GAShow all

10 papers · 2 filters

astro-ph.GA2019★ 45 cited

Effect of Electromagnetic Interaction on Galactic Center Flare Components

Arman Tursunov, Michal Zajaček, Andreas Eckart +5

Recently, near-infrared GRAVITY@ESO observations at have announced the detection of three bright "flares" in the vicinity of the Galactic center supermassive black…

astro-ph.GA2019★ 1 cited

Distribution of Radio Spectral Slopes of Galaxies in Optical Diagnostic Diagrams

Michal Zajaček, Andreas Eckart, Silke Britzen +1

For about 500 intermediate-redshift sources (), whose radio flux densities at are larger than 10 mJy, we performed additional observations at 4.85 GHz…

astro-ph.GA2019★ 2 cited

Quasars from LSST as dark energy tracers: first steps

Mary Loli Martínez-Aldama, Swayamtrupta Panda, Bożena Czerny +1

In the near future, new surveys promise a significant increase in the number of quasars (QSO) at large redshifts. This will help to constrain the dark energy models using quasars.…

astro-ph.GA2019

Modelling broad emission lines in active galactic nuclei

Bozena Czerny

Broad Emission Lines are the most characteristic features of Active Galaxies, but the mechanism of creating a medium able to emit these intense lines is not quite clear. Observatio…

astro-ph.GA2019★ 10 cited

Quasar Main Sequence: a line or a plane?

Conor Wildy, Bozena Czerny, Swayamtrupta Panda

A quasar main sequence is widely believed to reveal itself through objects represented in a plane spanned by two parameters: the full-width at half-maximum (FWHM) of H, and the…

astro-ph.GA2019★ 12 cited

Reverberation-mapping of distant quasars: time-lag determination using different methods

Michal Zajaček, Bożena Czerny, Mary-Loli Martinez Aldama +1

By applying different statistically robust methods, we analyze the time-lag between the continuum and ionized line-emission (Mg II line) light curves for the distant bright quasar…

astro-ph.GA2019

Slim accretion disks: theory and observational consequences

Bozena Czerny

Slim accretion disks idea emerged over 30 years ago as an answer to several unsolved problems. Since that time there was a tremendous increase in the amount of observational data w…

astro-ph.GA2019★ 12 cited

Mechanism of the Changing Look phenomenon in Active Galactic Nuclei

Marzena Śniegowska, Bożena Czerny

Changing-look phenomenon observed now in a growing number of active galaxies challenges our understanding of the accretion process close to a black hole. We propose a simple explan…

astro-ph.GA2019★ 13 cited

Stellar populations in hosts of giant radio galaxies and their neighbouring galaxies

Agnieszka Kuźmicz, Bożena Czerny, Conor Wildy

Context: Giant radio galaxies (with projected linear size of radio structure larger than 0.7 Mpc) are very rare and unusual objects. Only 5% of extended radio sources reach s…

astro-ph.GA2019★ 52 cited

Time delay measurement of Mg II line in CTS C30.10 with SALT

Bozena Czerny, Aleksandra Olejak, Mateusz Ralowski +18

We report 6 yr monitoring of a distant bright quasar CTS C30.10 (z = 0.90052) with the Southern African Large Telescope (SALT). We measured the rest-frame time-lag of da…