20 citations · 51 across the 3 of their papers we have counts for
4 papers
Ultraviolet Line Profiles of Slowly Rotating Massive Star Winds Using the "Analytic Dynamical Magnetosphere" Formalism
C. Erba, A. David-Uraz, V. Petit +6
Recent large-scale spectropolarimetric surveys have established that a small but significant percentage of massive stars host stable, surface dipolar magnetic fields with strengths…
Shock-heated radiation-driven outflows as a solution to the weak-wind problem of late O-type stars
C. Lagae, F. A. Driessen, L. Hennicker +2
Context. Radiation-driven mass loss is key to our understanding of massive-star evolution. However, for low-luminosity O-type stars there are big discrepancies between theoreticall…
A 3D short-characteristics method for continuum and line scattering problems in the winds of hot stars
L. Hennicker, J. Puls, N. D. Kee +1
Context: Knowledge about hot, massive stars is usually inferred from quantitative spectroscopy. To analyse non-spherical phenomena, the existing 1D codes must be extended to higher…
3D radiative transfer: Continuum and line scattering in non-spherical winds from OB stars
L. Hennicker, J. Puls, N. D. Kee +1
Context: State of the art quantitative spectroscopy of OB-stars compares synthetic spectra (calculated by means of 1D, spherically symmetric computer codes) with observations. Cert…