User profiles for Czerny, B.

Bozena Czerny

Center for Theoretical Physics
Verified email at cft.edu.pl
Cited by 11727

[HTML][HTML] Cosmology intertwined: A review of the particle physics, astrophysics, and cosmology associated with the cosmological tensions and anomalies

…, CJ Copi, F Courbin, FY Cyr-Racine, B Czerny…�- Journal of High Energy�…, 2022 - Elsevier
The standard Λ Cold Dark Matter (ΛCDM) cosmological model provides a good description
of a wide range of astrophysical and cosmological data. However, there are a few big open …

[HTML][HTML] Slim accretion disks

MA Abramowicz, B Czerny, JP Lasota…�- …�Journal, Part 1�…, 1988 - adsabs.harvard.edu
A new branch of equilibrium solutions for stationary accretion disks around black holes is
found. These solutions correspond to moderately super-Eddington accretion rates. The …

The role of stromal-derived factor-1—CXCR7 axis in development and cancer

…, J Tarnowska, M Wysoczynski, R Liu, B Czerny…�- European journal of�…, 2009 - Elsevier
Cancer metastasis is a major clinical problem that contributes to unsuccessful therapy.
Augmenting evidence indicates that metastasizing cancer cells employ several mechanisms that …

[HTML][HTML] Constraints on quasar accretion disks from the optical/ultraviolet/soft X-ray big bump

B Czerny, M Elvis�- Astrophysical Journal, Part 1 (ISSN 0004�…, 1987 - adsabs.harvard.edu
b) Comptonization In this case the classical description is not self-consistent and … ultraviolet
data; model B instead extends through to soft X-rays and produces the steep observed soft X-…

The origin of the broad line region in active galactic nuclei

B Czerny, K Hryniewicz�- Astronomy & Astrophysics, 2011 - aanda.org
Aims. Although broad emission lines are the most reliable signature of the nuclear activity of
a galaxy and the location of the emitting material is well measured by the reverberation …

Accretion disk model of short-timescale intermittent activity in young radio sources

B Czerny, A Siemiginowska, A Janiuk…�- The Astrophysical�…, 2009 - iopscience.iop.org
… The gas and radiation pressure are given by P gas = k B /m p ρT and P rad = 4/3σT 4 , whereτ
is the optical depth, Σ = ρH is the gas column density, c, k B, and σ are physical constants, …

Universal spectral shape of high accretion rate AGN

B Czerny, M Nikołajuk, A R�żańska…�- Astronomy &�…, 2003 - aanda.org
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 simple …

[HTML][HTML] Slim accretion disks: theory and observational consequences

B Czerny�- Universe, 2019 - mdpi.com
… , or might imply that in other sources the effect of winds and/or magnetic field changes the
regular outbursts into semi-regular periods of enhanced variability Janiuk and Czerny [42]. …

Vertical structure of the accreting two-temperature corona and the transition to an ADAF

A R�żańska, B Czerny�- arXiv preprint astro-ph/0004158, 2000 - arxiv.org
We investigate the model of the disc/corona accretion flow around the black hole. The model,
parameterized by the total (ie disk plus corona) accretion rate, $\dot m$, mass of the black …

Failed radiatively accelerated dusty outflow model of the broad line region in active galactic nuclei. I. Analytical solution

B Czerny, YR Li, K Hryniewicz, S Panda…�- The Astrophysical�…, 2017 - iopscience.iop.org
The physical origin of the broad line region in active galactic nuclei is still unclear despite
many years of observational studies. The reason is that the region is unresolved, and the …