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Astron. Astrophys. 356, 895-902 (2000) 2. Observations and reductionsThe photometric data have been gathered during three campaigns at
La Silla, Chile. For the A-component HD 220392, 7 nights of
measurements were made in June 1990, 11 nights were obtained in
September 1991 and 3 in October 1992. For the B-component
HD 220391, only observations made in September 1991 and October
1992 are available. The June 1990 and September 1991 campaigns have
been performed by P. Lampens with the Swiss 0.7m telescope of the
Geneva Observatory while the October 1992 data were obtained with the
ESO 0.5m telescope by D. Sinachopoulos. We have collected a
total of 396 data for the brightest component HD 220392 and 245
for HD 220391. The characteristics of these data are mentioned in
Table 1. Standard and additional programme stars have also been
observed during these nights. All Geneva measurements are absolute
measurements in the filters
UBVB1B2V1G obtained through a
centralized reduction scheme at the Geneva observatory (Rufener 1988).
This centralized Swiss processing has not been applied to the ESO data
taken in the UBV photometric system. The reduction of the October data
implied using a check-star HD 220729 [F4V, V=5.52, B-V=+0.40]
whose measurements were interpolated between the two other ones. We
have verified the constancy of this star in the Hipparcos catalogue
( Table 1. Photometric data for HD 220392 and HD 220391 ![]() ![]() ![]() ![]() © European Southern Observatory (ESO) 2000 Online publication: April 17, 2000 ![]() |