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B. Czerny

3 papers hereh-index 216 citations11 works total

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

author position
  • middle author1
  • last author2

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA2
  • astro-ph.HE1
same name
  • B. Czerny — 115 papers, h 39
  • B. Czerny — 18 papers
  • B. Czerny — 4 papers, h 6

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

most citedQuasar Main Sequence unfolded by 2.5D FRADO (Natural expression of Eddington ratio, black hole mass, and inclination)

2 citations · 2 across the 2 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2026

Radiation-pressure instability is an artifact of constant-α closure. Implications for AGN disk tensions

M. H. Naddaf, M. Ghasemnezhad, H. Ghanbarnejad +2

The standard α-disk formalism parametrizes turbulent angular momentum transport through a dimensionless coefficient α, assumed to be spatially and thermodynamically invariant.…

astro-ph.GA2025★ 2 cited

Quasar Main Sequence unfolded by 2.5D FRADO (Natural expression of Eddington ratio, black hole mass, and inclination)

M. H. Naddaf, M. L. Martínez-Aldama, P. Marziani +2

The quasar main sequence (QMS), characterized by the Eigenvector 1 (EV1), serves as a unifying framework for classifying type-1 active galactic nuclei (AGNs) based on their diverse…

astro-ph.GA2025

Hβ line shape and radius-luminosity relation in 2.5D FRADO

M. H. Naddaf, M. L. Martinez-Aldama, D. Hutsemekers +2

Galaxies with active galactic nuclei (AGN) exhibit broad emission lines as a key spectral feature. The shape of emission-line profiles depends on the complex dynamics of discrete c…

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