Stellar populations with adaptive optics: four test cases.

Physics – Optics

Scientific paper

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Galaxies: Stellar Populations

Scientific paper

The authors have made a first attempt to apply adaptive optics to the study of stellar populations in our Galaxy and beyond. In the cases of NGC 5128 and IC 5152, they failed to detect individual stars. For NGC 300 the authors resolved a small number of K supergiants in the disk. For the Sgr bulge window the colour-magnitude diagram and luminosity function are the deepest yet obtained, reaching the turnoff of the bulge population for the first time in the infrared. These results demonstrate the feasibility of the method.

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