19 citations · 38 across the 4 of their papers we have counts for
4 papers
Radiation-driven winds of hot luminous stars. XVIII. The reliability of stellar and wind parameter determinations from spectral analysis of selected central stars of planetary nebulae and the possibility of single-star SN Ia progenitors
C. B. Kaschinski, A. W. A. Pauldrach, T. L. Hoffmann
Context. The uncertainty in the degree to which radiation-driven winds of hot stars might be affected by small inhomogeneities in the density leads to a corresponding uncertainty i…
Effects of shocks in stellar atmosphere models on the emission line spectrum of surrounding Hii regions
C. B. Kaschinski, Barbara Ercolano
Emission line studies from Hii regions in galaxies require tools for the inversion of line ratios into desired physical properties. These tools generally come in form of diagnostic…
Radiation-driven winds of hot luminous stars XVII. Parameters of selected central stars of PN from consistent optical and UV spectral analysis and the universality of the mass-luminosity relation
C. B. Kaschinski, A. W. A. Pauldrach, T. L. Hoffmann
Context: The commonly accepted mass-luminosity relation of central stars of planetary nebulae (CSPNs) might not be universally valid. While earlier optical analyses could not deriv…
Spectroscopic Constraints on the Form of the Stellar Cluster Mass Function
N. Bastian, I. S. Konstantopoulos, G. Trancho +5
This contribution addresses the question of whether the initial cluster mass function (ICMF) has a fundamental limit (or truncation) at high masses. The shape of the ICMF at high m…