Physics
Scientific paper
Jul 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995hst..prop.6284w&link_type=abstract
HST Proposal ID #6284
Physics
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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