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Astron. Astrophys. 332, 939-957 (1998)

Footnotes

1. Based on data obtained in observing time allocated by Mc Donald Observatory, Texas; Mauna Kea Observatory, Hawaii; Vainu Bappu Observatory, India; Wise Observa- tory, Israel; Haute-Provence Observatory, France; The Nordic Optical Telescope and the Isaac Newton Telescope at Roque de Los Muchachos Observatory, La Palma, Spain

2. AM CVn was included in the Carlsberg Meridian Circle programme at La Palma in 1992 and 1993. The first year it was constant, while it in 1993 varied between [FORMULA] and 13.7 (Solheim 1995)

3. The unit mi refers to the fractional intensity (on a linear scale) relative to the mean brightness of the star. 100 per cent modulation is by definition 1 mi = 1000 mmi

© European Southern Observatory (ESO) 1998

Online publication: March 30, 1998
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