Preface | p. 1 |
List of participants | p. 3 |
Massive stars: setting the stage | p. 7 |
The massive star distribution in the Galaxy and the Magellanic Clouds | p. 21 |
Massive star distribution in external galaxies and starburst regions | p. 37 |
Dissection of 30 Doradus and a discussion of the Magellanic Cloud OB-associations | p. 55 |
Blue and red supergiants and the age structure of the NGC 330 region | p. 61 |
Stars in young clusters in the Magellanic Clouds | p. 65 |
The population of massive stars in R136 from HST/FOC UV observations | p. 69 |
Spectral synthesis of spectral populations using Balmer lines | p. 75 |
The stellar content of the Orion OB1 association | p. 81 |
Observations of the atmospheres and winds of O-stars, LBV's and Wolf-Rayet stars | p. 85 |
Radiation driven winds of hot stars: theory of O-star atmospheres as a spectral tool | p. 105 |
The chemical composition of B-supergiant atmospheres | p. 127 |
Intrinsic parameters of massive OB-stars | p. 137 |
Line blanketing by iron group elements in non-LTE model atmospheres of hot stars | p. 147 |
A comparison between observed and predicted mass loss rates and wind momentum of O stars | p. 153 |
LTE and NLTE abundances in A supergiants: a test of their evolutionary status | p. 163 |
A spectroscopic analysis of B-stars in the SMC cluster NGC 330 | p. 169 |
Hydrodynamic atmosphere models for hot luminous stars II. Method and improvements over unified models | p. 173 |
Hubble space telescope spectroscopy of massive hot stars in the Magellanic Clouds and M31 | p. 179 |
Stellar winds of massive stars in M31 | p. 183 |
O-star winds in the Magellanic Clouds and the Milky Way | p. 187 |
On the relation between the mass loss rate and the stellar parameters of OB-type stars | p. 191 |
Wind asymmetries in massive stars | p. 193 |
NLTE analysis of hot binaries | p. 199 |
Effective temperatures and surface gravities of early type stars | p. 203 |
The atmospheric composition, extinction and luminosity of the LBV star R71 | p. 207 |
The variability of Eta Car: a tool for the LBV phenomenon | p. 211 |
The nature of the luminous blue variable AG Car | p. 215 |
The evolutionary status of Eta Car based on historical and modern optical and infrared photometry | p. 219 |
The gradual acceleration of the outflow of VX Sagittari; a stellar evolution effect? | p. 225 |
The complex H-alpha profile of the hypergiant HR 8752 during 1970-1992 | p. 231 |
Spectral analysis of Wolf-Rayet stars: theory, results, conclusions | p. 237 |
Line-blanketed non-LTE atmosphere models for Wolf-Rayet stars | p. 253 |
The fundamental parameters of the central stars of eight WR ring nebulae | p. 263 |
Tailored analysis of 24 galactic WN stars | p. 271 |
Oxygen and carbon abundances for the WO stars | p. 277 |
HD190918: arbiter between models for Wolf-Rayet stars | p. 281 |
Structure and evolution of massive stars: mixing processes and stellar evolution | p. 285 |
Overshooting from convective cores: theory and numerical simulation | p. 299 |
Massive close binaries, observational characteristics | p. 309 |
Doppler tomography of O-type binaries; the physical properties of seven systems | p. 323 |
Evolution of massive close binaries | p. 327 |
Massive single star evolution: comparison with observations | p. 349 |
Presupernova evolution of the most massive stars | p. 365 |
Properties of massive star evolution | p. 373 |
Nucleosynthesis in massive stars | p. 383 |
Results of evolutionary computations of primaries of close binaries with different initial composition | p. 391 |
The mass and helium discrepancy in massive stars: the case Vela X-1 | p. 395 |
On the evolution of secondary components in massive close binary systems | p. 401 |
Double-zone model with diffusive mixing and the mass and helium discrepancies in OB stars | p. 405 |
The impact of semi-convection and overshooting on the surface abundances in massive stars | p. 409 |
Improved bolometric corrections for WR stars | p. 413 |
Wolf-Rayet stars in starbursts | p. 417 |
A study of the SMC cluster NGC330 | p. 421 |
The evolution of massive stars to explosion | p. 425 |
SN1987A and SN1993J: testing stellar evolution theory | p. 439 |
Chemical and photometric evolution of elliptical galaxies | p. 455 |
A model for the chemical evolution of the solar neighborhood using metallicity dependent yields | p. 471 |
Poster list | p. 477 |
Summary | p. 485 |
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