Showing 1–20 of 28 results
/ Date/ Name
Jul 2, 2003Radiation-driven winds of hot luminous stars. XV. Constraints on the mass-luminosity relation of central stars of planetary nebulaeDec 10, 2002Hot Stars: Old-Fashioned or Trendy?Oct 23, 2018Numerical Models for the Diffuse Ionized Gas in Galaxies. II. Three-dimensional radiative transfer in inhomogeneous interstellar structures as a tool for analyzing the diffuse ionized gasJul 4, 2011Radiation-driven winds of hot luminous stars. XVI. Expanding atmospheres of massive and very massive stars and the evolution of dense stellar clustersSep 18, 2001Gravitationally lensed high redshift galaxies in the field of 1E0657-56Jan 13, 2000Spectra of High Redshift Galaxies using a Cluster as a Gravitational TelescopeJun 2, 2012Numerical Models for the Diffuse Ionized Gas in Galaxies. I. Synthetic spectra of thermally excited gas with turbulent magnetic reconnection as energy sourceJul 11, 2013Non-LTE models for synthetic spectra of type Ia supernovae. IV. A modified Feautrier scheme for opacity-sampled pseudo-continua at high expansion velocities and application to synthetic SN Ia spectraApr 24, 2002Model atmospheres for type Ia supernovae: Basic steps towards realistic synthetic spectraOct 29, 2004Consistent Radiative Transfer Models including Time Dependent Energy Deposition for Type Ia SupernovaeAug 24, 2006Non-LTE models for synthetic spectra of type Ia supernovae/hot stars with extremely extended atmospheresJul 11, 2013Non-LTE models for synthetic spectra of type Ia supernovae. III. An accelerated lambda iteration procedure for the mutual interaction of strong spectral lines in SN Ia models with and without energy depositionJul 10, 2013Radiation-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 progenitorsFeb 28, 2007Central stars of planetary nebulae in the Galactic bulgeMar 30, 2005The VLT-FLAMES Survey of Massive Stars: Observations in the Galactic Clusters NGC 3293, NGC 4755 and NGC 6611Apr 17, 2013Three-Dimensional Modelling of Ionized Gas. I. Did very massive stars of different metallicities drive the second cosmic reionization?Mar 22, 2005The 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 SampleFeb 26, 2004The Physical Properties and Effective Temperature Scale of O-type Stars as a Function of Metallicity. I. A Sample of 20 Stars in the Magellanic CloudsJan 21, 2015Three-dimensional modeling of ionized gas. II. Spectral energy distributions of massive and very massive stars in stationary and time-dependent modeling of the ionization of metals in HII regionsApr 5, 2012Radiation-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