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The All Sky Automated Survey (ASAS) data, covering nearly 70% of the wholesky south of declination +28 deg, were recently used to discover about 300 BetaCephei stars brighter than V~11.5 mag. As this means a nearly fourfold increasein the number of known stars of this type, new possibilities in studying thesepulsators open up, including statistical work. The homogeneity of the ASASsurvey allows us to study their distribution in the local Galaxy. We discussthis distribution in the context of the location of nearby spiral arms. Inaddition, we show pulsational (periods, amplitudes) properties of the wholesample of known Beta Cephei stars. Some objects interesting from the point ofview of asteroseismology are also indicated.

Beta Cephei stars from ASAS: a new look at hot pulsators