Stellar Populations in the Local Group

Physics

Scientific paper

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Hst Proposal Id #6284 Stellar Populations

Scientific paper

In Cycle 4 we obtained WFPC2 images of a portion of the OB association NGC 206 in M31 for the purpose of determining the Initial Mass Function of the intermediate mass stars. In this program we are obtaining a background field in order to be able to subtract, statistically, stars in the NGC 206 field that are not members of the association. This is necessary in order to determine a true IMF of the association.

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