Follow-up observations of the DSCT V350 Peg

Physics

Scientific paper

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Scientific paper

We present all the CCD photometric observations of the Delta Scuti star V350~Peg performed by us until now. The data have been acquired between 1997 July and 2002 October. A large part has been analysed and presented previously (Vidal 2002a). The new data of 2002 confirm the former conclusion that two frequencies of very similar amplitudes are excited in this star. The entire data set consists of 16191 measurements collected during 48 nights, and may be very helpful to investigate the detailed behaviour of this basically double-mode Delta Scuti variable if future campaigns are held at a later stage.

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