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researcher

W. Kluźniak

124 papers hereh-index 4410.8k citations270 works total

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

author position
  • sole author5
  • first author9
  • middle author37
  • last author25

Across the 76 of 124 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE69
  • astro-ph41
  • astro-ph.SR5
  • gr-qc4
  • astro-ph.IM3
  • astro-ph.CO1
same name
  • W. Kluźniak — 89 papers, h 33
  • W. Kluźniak — 22 papers, h 8
  • W. Kluźniak — 12 papers
  • W. Kluźniak — 12 papers, h 2
  • W. Kluźniak — 8 papers, h 7
  • W. Kluźniak — 7 papers, h 3

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
19972023
most citedSearch for dark matter annihilations towards the inner Galactic halo from 10 years of observations with H.E.S.S

314 citations · 5.3k across the 121 of their papers we have counts for

collaborators
Showing 2009Show all

3 papers · 1 filter

astro-ph.HE2009★ 243 cited

Radio Imaging of the Very-High-Energy Gamma-Ray Emission Region in the Central Engine of a Radio Galaxy

The VERITAS Collaboration, the VLBA 43 GHz M 87 Monitoring Team, the H. E. S. S. Collaboration +1

The accretion of matter onto a massive black hole is believed to feed the relativistic plasma jets found in many active galactic nuclei (AGN). Although some AGN accelerate particle…

astro-ph.HE2009★ 20 cited

Global transient dynamics of three-dimensional hydrodynamical disturbances in a thin viscous accretion disk

Paola Rebusco, Orkan M. Umurhan, Wlodek Kluzniak +1

Thin viscous Keplerian accretion disks are considered asymptotically stable, even though they can show significant dynamic activity on short timescales. In this paper the dynamics…

astro-ph.HE2009★ 20 cited

Vertical dissipation profiles and the photosphere location in thin and slim accretion disks

A. Sadowski, M. Abramowicz, M. Bursa +2

We calculate optically thick but geometrically thin (and slim) accretion disk models and perform a ray-tracing of photons (in the Kerr geometry) to calculate the observed disk spec…

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