CCD photometry of YY Orionis stars (Harder+ 1998)

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Photometry: Ubvri, Stars: Pre-Main Sequence, Stars: Variable

Scientific paper

Results of photometric monitoring in the UBVRI bands of 5 YY Orionis stars and 2 other variable stars are presented. Each source was observed in the period of 1996, Nov. 23 to Dec. 2 and of 1996, Dec. 23 to 1997,Jan. 2 at the 1-m telescope of Wise Observatory, Israel. Tables.dat contain the luminosity variation of each star as deviation from its average observed magnitude. (1 data file).

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