Salpeter mass functions of young populous clusters in the LMC?

Physics

Scientific paper

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Color-Magnitude Diagram, Magellanic Clouds, Mass To Light Ratios, Star Clusters, Stellar Mass, Early Stars, Stellar Luminosity

Scientific paper

Photometry was used to study several young LMC clusters and to test the
proposition that the IMF of stars in such clusters has a universal
shape. The proposition is not proved or refuted here, but it is shown
that the very steep IMFs found by Mateo (1989) are not real but probably
result from a special aspect of his data reduction.

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