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researcher

L. M. Oskinova

4 papers here

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

author position
  • first author2
  • middle author1
  • last author1

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

fields
  • astro-ph.SR2
  • astro-ph1
  • astro-ph.GA1
ORCID 0000-0003-0708-4414

identity via Semantic Scholar / OpenAlex

activity
20082015
most citedThe Quintuplet Cluster III. Hertzsprung-Russell diagram and cluster age

43 citations · 59 across the 4 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

2 papers · 1 filter

astro-ph.SR2015★ 11 cited

On X-ray pulsations in beta Cephei-type variables

L. M. Oskinova, H. Todt, D. P. Huenemoerder +4

Beta Cephei-type variables are early B-type stars that are characterized by oscillations observable in their optical light curves. At least one Beta Cep-variable also shows periodi…

astro-ph.SR2012★ 2 cited

3-D Monte Carlo radiative transfer calculation of resonance line formation in the inhomogeneous expanding stellar wind

Brankica Šurlan, Wolf-Rainer Hamann, Jiří Kubát +2

We study the effects of optically thick clumps, non-void inter-clump medium, variation of the onset of clumping, and velocity dispersion inside clumps on the formation of resonance…

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