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L. M. Oskinova

4 papers here

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

author position
  • first author3
  • last author1

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

fields
  • astro-ph3
  • astro-ph.SR1
ORCID 0000-0003-0708-4414

identity via Semantic Scholar / OpenAlex

most citedThe Quintuplet Cluster I. A K-band spectral catalog of stellar sources

63 citations · 110 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2009★ 34 cited

Discovery of X-ray Emission from the Wolf-Rayet star WR142 of oxygen subtype

L. M. Oskinova, W. -R. Hamann, A. Feldmeier +2

We report the discovery of weak yet hard X-ray emission from the Wolf-Rayet (WR) star WR142 with the XMM-Newton X-ray telescope. Being of spectral subtype WO2, WR142 is a massive s…

astro-ph2008★ 63 cited

The Quintuplet Cluster I. A K-band spectral catalog of stellar sources

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

Three very massive clusters are known to reside in the Galactic Center region, the Arches cluster, the Quintuplet cluster and the Central parsec cluster. We obtained spectroscopic…

astro-ph2008★ 10 cited

Puzzling X-rays from the new colliding wind binary WR65

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

We report the discovery of variability in the X-ray emission from the Wolf-Rayet type star WR 65. Using archival Chandra data spanning over 5 yr we detect changes of the X-ray flux…

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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