L. Oskinova

Astronomy and Astrophysics · 2007–2014

A researcher in the Science corpus: 2 papers; trusts 10 researchers and is trusted by 5 researchers here, as inferred from the citation graph.

Subfields

Whom L. Oskinova trusts overall

Their strongest outbound trust, strongest first, inferred from their citations.

  1. S. Owocki
  2. J. Puls
  3. A. Fullerton
  4. W. Hamann
  5. D. Massa
  6. P. Crowther
  7. Philip Massey
  8. G. Gräfener
  9. R. Kudritzki
  10. N. Markova

Who trusts L. Oskinova overall

  1. M. Gudel
  2. J. Puls
  3. Y. Nazé
  4. J. Vink
  5. Roland Walter

Papers from L. Oskinova's perspective

Ordered by how strongly the researchers L. Oskinova trusts endorse each paper. Same corpus, a different order for every researcher.

  1. Lower mass loss rates in O-type stars: Spectral signatures of dense clumps in the wind of two Galactic O4 stars
  2. WINDS FROM HOT STARS
  3. The Discordance of Mass-Loss Estimates for Galactic O-Type Stars
  4. The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 M⊙ stellar mass limit
  5. The outer evolution of instability-generated structure in radiatively driven stellar winds
  6. Stellar and wind properties of LMC WC4 stars A metallicity dependence for Wolf-Rayet mass-loss rates ?
  7. The Physical Properties and Effective Temperature Scale of O-Type Stars as a Function of Metallicity. II. Analysis of 20 More Magellanic Cloud Stars and Results from the Complete Sample
  8. Presupernova Evolution of Rotating Massive Stars. II. Evolution of the Surface Properties
  9. A Porosity-Length Formalism for Photon-Tiring-limited Mass Loss from Stars above the Eddington Limit
  10. Stellar evolution with rotation XI. Wolf-Rayet star populations at different metallicities

Their papers