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B. Šurlan

1 paper here

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

author position
  • first author1

Across the 1 of 1 paper where every author was matched, so the position is known.

fields
  • astro-ph.SR1
same name
  • B. Šurlan — 3 papers, h 3
  • B. Šurlan — 1 paper

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

most cited3-D radiative transfer in clumped hot star winds I. Influence of clumping on the resonance line formation

79 citations · 79 across the 1 of their papers we have counts for

collaborators

1 paper

astro-ph.SR2012★ 79 cited

3-D radiative transfer in clumped hot star winds I. Influence of clumping on the resonance line formation

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

The true mass-loss rates from massive stars are important for many branches of astrophysics. For the correct modeling of the resonance lines, which are among the key diagnostics of…

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