Date Presented:

2006/08/1

Abstract:

We report on the results of a series of photometric observations of the low-amplitude δ Scuti star GSC 4778:0324, in the course of a multi-site campaign aiming at monitoring V1162 Ori. The two dominant frequencies, found in the previous analyses based on the 2000-2002 data, are confirmed and their amplitudes are found to be stable on a time-scale of a few years.

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