Physics
Scientist
Amsterdam, Universiteit, Netherlands
Brussel, Vrije Universiteit, Brussels, Belgium
An evolutionary scenario for the black hole binary A0620-00
An Operational Concept for a Small Autonomous Satellite
Evolution of low-mass close binary sytems with a compact mass accreting component
Magnetic structure in cool stars. XV - The evolution of rotation rates and chromospheric activity of giants
The combined effect of mass loss and overshooting. V - Massive stars in the Magellanic Clouds
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