activity
20002020
most citedEvolution of the X-ray spectrum in the flare model of Active Galactic Nuclei

45 citations · 262 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.GA2020★ 12 cited

The multi-phase environment in the centre of Centaurus A

A. Borkar, T. P. Adhikari, A. Różańska +6

We study the multi-phase medium in the vicinity of the active galactic nucleus Centaurus A (Cen A). Combined high-resolution observations with the ALMA and Chandra observatories in…

astro-ph.HE2020★ 12 cited

Accurate Treatment of Comptonization in X-ray Illuminated Accretion Disks

Javier A. García, Ekaterina Sokolova-Lapa, Thomas Dauser +5

A large fraction of accreting black hole and neutron stars systems present clear evidence of the reprocessing of X-rays in the atmosphere of an optically-thick accretion disk. The…

astro-ph.HE2019★ 28 cited

Incoherent fast variability of X-ray obscurers. The case of NGC 3783

B. De Marco, T. P. Adhikari, G. Ponti +22

Context. Obscuration events caused by outflowing clumps or streams of high column density, low ionisation gas, heavily absorbing the X-ray continuum, have been witnessed in a numbe…

astro-ph.HE2019★ 29 cited

The high energy universe at ultra-high resolution: the power and promise of X-ray interferometry

Phil Uttley, Roland den Hartog, Cosimo Bambi +24

We propose the development of X-ray interferometry (XRI), to reveal the universe at high energies with ultra-high spatial resolution. With baselines which can be accommodated on a…

astro-ph.HE2019★ 19 cited

Orientation of the crescent image of M 87*

Krzysztof Nalewajko, Marek Sikora, Agata Różańska

The first image of the black hole (BH) M 87* obtained by the Event Horizon Telescope (EHT) has the shape of a crescent extending from the E to WSW position angles, while the observ…

astro-ph.HE2019★ 40 cited

Warm and thick corona for magnetically supported disk in GBHB

Dominik Gronkiewicz, Agata Różańska

This paper is devoted to self-consistent modeling of the magnetically supported accretion disk with optically thick warm corona based on first principles. In our model, we consider…