Coordinated investigation of selected regions in the Magellanic Clouds.

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

The greatly enhanced observational Possibilities for research in the Magellanic Clouds, such as bigger telescopes and the CCD as detector, has led the way to studies hitherto unimagined. The possibility to reach 60 kpc distant stars of fifth absolute magnitude (i. e. down to main-sequence stars fainter than the Sun) or to obtain stellar spectra to do a fine-analysis of atmospheric temperature and composition has mightily raised the importance of the astrophysical laboratory called Magellanic Clouds. In particular the study of the intricately interwoven processes of formation of stars from progenitor gas clouds and the evolution of stellar complexes can in our times superbly be investigated by observing the Magellanic Cloud constituents.

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