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V. Karas

4 papers hereh-index 5129 citations10 works total

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

author position
  • sole author1
  • middle author2

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph2
  • astro-ph.HE1
  • gr-qc1
same name
  • V. Karas — 303 papers, h 41
  • V. Karas — 29 papers, h 17
  • V. Karas — 15 papers, h 12
  • V. Karas — 10 papers, h 11
  • V. Karas — 9 papers
  • V. Karas — 7 papers, h 9

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
20042026
most citedStar-disc interactions in a galactic centre and oblateness of the inner stellar cluster

22 citations · 24 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2026

A secondary orbiter under collisions with an accretion disk

Vladimir Karas

Dynamics of stellar orbits in dense stellar systems and nuclear star clusters (NSC) with an embedded supermassive black hole (SMBH) is governed a complex interplay of different for…

gr-qc2020★ 2 cited

The exterior gravitational potential of toroids

J. -M. Huré, B. Basillais, V. Karas +2

We perform a bivariate Taylor expansion of the axisymmetric Green function in order to determine the exterior potential of a static thin toroidal shell having a circular section, a…

astro-ph2005

X-ray Variability of Active Galactic Nuclei and the Flare Model

R. W. Goosmann, B. Czerny, A. -M. Dumont +4

Short-term variability of X-ray spectra has been reported for several Active Galactic Nuclei. Significant X-ray flux variations are observed within time scales down to 10^4 -- 10^5…

astro-ph2004★ 22 cited

Star-disc interactions in a galactic centre and oblateness of the inner stellar cluster

L. Subr, V. Karas, J. -M. Hure

Structure of a quasi-stationary stellar cluster is modelled assuming that it is embedded in the gravitational field of a super-massive black hole. Gradual orbital decay of stellar…

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