Asteroseismology in the young open cluster NGC 3293

Details Asteroseismology in the young open cluster NGC 3293 Asteroseismology in the young open cluster NGC 3293

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008coast.157..315h&link_type=abstract

Communications in Asteroseismology, Vol.157, p. 315-316

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Scientific paper

This is a progress report on the analysis of our extensive CCD UBV photometry campaign of the open cluster NGC 3293 that contains eleven known β Cephei stars. All of them are multiperiodic with up to seven independent mode periods detected so far. Another group of variables is located near the low-luminosity end of the β Cephei instability strip; it probably consists of rapidly rotating SPB stars. More than a dozen δ Scuti stars have been confidently identified in the field so far. All are new discoveries; about half of them belong to the cluster. To date, we have also discovered five eclipsing variables in and around NGC 3293.

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