New periods of variable stars in Cygnus based on a quarter of century of photographic observations*
Astronomical Institute of the Slovak Academy of Sciences, 059 60 Tatranská Lomnica, The Slovak Republic e-mail: email@example.com firstname.lastname@example.org
Send offprint request to: L. Hric
Accepted: 22 September 1998
This work summarizes the results of photographic photometry obtained over 24 years at the Skalnaté Pleso (1979-1993) and Asiago (1969-1988) observatories. The period of light changes, the epoch of the maximum or of the minimum, the type of variability and, in some cases, possible causes of the long-term behaviour of light changes were determined for 17 variable stars.
Key words: stars: techniques: photometric / stars: variables: general
Tables 2 is only and Table 3 also available at the CDS via anonymous ftp 220.127.116.11 and http://cdsweb.u-strasbg.fr/Abstract.html
© European Southern Observatory (ESO), 1999