The STACC 1998 campaign on BN CNC The Paesepe cluster

Details The STACC 1998 campaign on BN CNC The Paesepe cluster The STACC 1998 campaign on BN CNC The Paesepe cluster

Jul 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997dssn...11....6f&link_type=abstract

Delta Scuti Star Newsletter, Issue 11, p. 6

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Scientific paper

Stellar modelling has developed a lot in recent years thanks to the attempts to model the Sun well enough to remove discrepancies with helioseismic data and to explain a few outstanding problems in variable star research (double mode Cepheids, the instability of Beta Cephei stars). We want to meet this theoretical challenge in terms of observations of a quality that equal the improved quality of stellar modelling. The target is the nearby open cluster Praesepe, which has a rich population of Delta Scuti stars that have been extensively observed. As target we prefer BN Cnc, which has bright star BV Cnc (see later) nearby that serves as a good reference. The other Delta Scuti variables with rich sets of pulsation modes in this cluster do not offer as nice a field of view for CCD photometry.

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