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researcher

B. Czerny

151 papers hereh-index 395.8k citations335 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author4
  • first author15
  • middle author76
  • last author32

Across the 127 of 151 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA51
  • astro-ph49
  • astro-ph.HE39
  • astro-ph.CO11
  • astro-ph.IM1
same name
  • B. Czerny — 6 papers, h 6
  • B. Czerny — 6 papers, h 2
  • B. Czerny — 5 papers

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19972026
most citedRadiation spectra of warm and optically thick coronae in AGN

99 citations · 1.3k across the 87 of their papers we have counts for

collaborators
Showing 2003 · astro-phShow all

4 papers · 2 filters

astro-ph2003

On the turbulent α-disks and the intermittent activity in AGN

Agnieszka Janiuk, Bozena Czerny, Aneta Siemiginowska +1

We consider effects of the MHD turbulence on the viscosity during the evolution of the thermal-viscous ionization instability in the standard α-accretion disks. We consider the p…

astro-ph2003

The origin of emission and absorption features in Ton S180 Chandra observations

A. Różańska, B. Czerny, A. Siemiginowska +2

We present new interpretation of Ton S180 spectrum obtained by {\it Chandra} Spectrometer (Low Energy Transmission Grating). Several narrow absorption lines and a few emission disk…

astro-ph2003

Universal spectral shape of AGN with high accretion rate

M. Nikolajuk, B. Czerny, A. Rozanska +1

The spectra of radio quiet and NLS1 galaxies show suprising similarity in their shape. They seem to scale only with the accretion rate but not with central black hole mass. We cons…

astro-ph2003

Universal spectral shape of high accretion rate AGN

B. Czerny, M. Nikolajuk, A. Rozanska +3

The spectra of quasars and NLS1 galaxies show surprising similarity in their spectral shape. They seem to scale only with the accretion rate. This is in contradiction with the simp…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.