The derived binary fraction of early-type stars is different for
individual star forming regions, suggesting a connection with the age and
the environment conditions. The few studies that have investigated this
connection do not provide conclusive results. To fill in this gap, we
started a detailed adaptive-optic-assisted imaging survey of early-type
field stars to derive their multiplicity in a homogeneous way. The sample
has been extracted from the Hipparcos Catalog and consists of 341 BA-type
stars within 300 pc from the Sun. We report the current status of the survey and describe a Monte-Carlo simulation that estimates the
completeness of our companion detection. Finally, the first results from
our second epoch observations of stars with companion candidates are
discussed.