The chemical composition of stars in open clusters.

Astronomy and Astrophysics – Astronomy

Scientific paper

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Stellar Spectra, Stars:Temperatures, Stars:Chemical Composition

Scientific paper

Until now few high-dispersion spectra have been obtained of stars in galactic star clusters and most of the spectra are of giant and supergiant stars that are very difficult to analyse. To reach fainter clusters and intrinsically fainter (main-sequence) stars in the nearer clusters, more photons are necessary. This is exactly the great advantage of the VL T, and Dr. Poul Erik Nissen of the AstronomicalInstitute in Aarhus, Denmark, explains how he would like to carry out such a programme.

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