We discuss observations and seismic analyses for three multi-periodic
delta Scuti stars in the Praesepe cluster: BU, BN and BV Cnc. For two
stars (BU and BN Cnc) we re-analyse published photoelectric photometry
and show that using statistical weights results in a dramatic reducti
on in the noise level. We detect seven frequencies in BU Cnc and eight
in BN Cnc, with three of the latter being previously unknown. We also
present new time-series CCD observations of BN and BV Cnc that succes
sfully demonstrate high-precision differential photometry on strongly
defocussed images. The observations show that BV Cnc is a multi-period
ic variable, with at least four oscillation frequencies. Finally, we c
ompare the observed oscillation frequencies in the three stars with mo
dels and derive luminosities, effective temperatures and masses.