Abstract
Between 1972 and 1990, in the course of the Hvar-Ondřejov photometric monitoring of bright northern Be stars, about 14 000 UBV measurements were secured for 76 objects (Pavlovski et al. 1997). We used the Hvar archival data (Harmanec et al. 1997) to study the incidence and characteristics of variability patterns for 48 Be stars with good time coverage.
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Pavlovski, K., Harmanec, P., Bozié, H., et al. (1997): AAS 125, 75
Harmanec, P., Pavlovski, K., Bozié, H., et al. (1997): J. Astron. Data (in press)
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© 1998 Springer-Verlag Berlin Heidelberg
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Pavlovski, K., Ružić, Ž., Dominis, D. (1998). The Interrelation Between Long-Term Cycles and Rapid Variations in Be Stars: A Photometric View. In: Kaper, L., Fullerton, A.W. (eds) Cyclical Variability in Stellar Winds. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-68597-5_34
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DOI: https://doi.org/10.1007/978-3-540-68597-5_34
Publisher Name: Springer, Berlin, Heidelberg
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