Red stars in nearby galaxies.

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Cool Stars:Magellanic Clouds, Galaxies:Evolution, Galaxies:Red Stars

Scientific paper

The study of the very cool stars in our Galaxy and in other galaxies is of great importance for our understanding of galaxy evolution. The first step in such an investigation is to identify these stars among the numerous warmer ones. Various search techniques are available and are here described by Professor Bengt Westerlund from the Uppsala Observatory in Sweden and formerly ESO Director in Chile. In particular, the new GRISMs at the prime focus of the 3.6 m telescope allow the detection of even very faint M, C and S stars. The extremely promising results of the initial observations are discussed by the author.

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