◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

W. Hamann

3 papers here

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

author position
  • middle author1
  • last author1

Across the 2 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph3

identity via Semantic Scholar / OpenAlex

most citedNeglecting the porosity of hot-star winds can lead to underestimating mass-loss rates

204 citations · 204 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph2008

A new outburst in LMC-N66

Miriam Pena, M. Teresa Ruiz, Patricio Rojo +2

This is the first report on the new outburst presented by the central star of the LMC-N66 nebula. This object was classified as a planetary nebula, however, its true nature is unde…

astro-ph2007

Determining element abundances of [WC]-type Central Stars for probing stellar evolution and nucleosynthesis

H. Todt, M. Peña, W. -R. Hamann +1

[WC]-type CSPNs are hydrogen-deficient Central Stars of Planetary Nebulae showing strong stellar winds and a carbon-rich chemistry. We have analyzed new high-resolution spectra of…

astro-ph2007★ 204 cited

Neglecting the porosity of hot-star winds can lead to underestimating mass-loss rates

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

Context: The mass-loss rate is a key parameter of massive stars. Adequate stellar atmosphere models are required for spectral analyses and mass-loss determinations. Present models…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.