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L. M. Oskinova

2 papers here

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

author position
  • first author1
  • middle author1

Across the 2 of 2 papers where every author was matched, so the position is known.

fields
  • astro-ph1
  • astro-ph.SR1
ORCID 0000-0003-0708-4414

identity via Semantic Scholar / OpenAlex

most citedAnalysis of the WN star WR 102c, its WR nebula, and the associated cluster of massive stars in the Sickle Nebula

8 citations · 11 across the 2 of their papers we have counts for

collaborators

2 papers

astro-ph.SR2016★ 8 cited

Analysis of the WN star WR 102c, its WR nebula, and the associated cluster of massive stars in the Sickle Nebula

M. Steinke, L. M. Oskinova, W. -R. Hamann +3

The massive Wolf-Rayet type star WR 102c is located near the Quintuplet Cluster - one of the three massive star clusters in the Galactic Center region. Previous studies indicated t…

astro-ph2008★ 3 cited

X-raying clumped stellar winds

L. M. Oskinova, W. -R. Hamann, A. Feldmeier

X-ray spectroscopy is a sensitive probe of stellar winds. X-rays originate from optically thin shock-heated plasma deep inside the wind and propagate outwards throughout absorbing…

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