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The study of massive stars can help us to understand how the universe has evolved to its current state, as these environments resemble the conditions of the time when the universe was still young. Frank Tramper provides a detailed analysis of such massive stars, which are located in galaxies beyond our own Milky Way, and its two satellite dwarf galaxies, the Magellanic Clouds.

Event details of The properties of low-metallicity massive stars
Date 28 November 2014
Time 12:00 -13:00
Location Agnietenkapel

F. Tramper, The Properties of Low-metallicity Massive Stars.

Supervisors

Prof. A. de Koter
Prof. L. Kaper

Co-supervisor

Dr H Sana

Agnietenkapel

Oudezijds Voorburgwal 229 - 231
1012 EZ Amsterdam

Entrance

This event is open to the public.