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Astron. Astrophys. 324, 357-365 (1997)

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Acknowledgements

We are grateful to Jose Ruedas at the Instituto de Astrofisica de Andalucia for helping us read two corrupted data files. We are also grateful to H. Schleicher and A. Fitzsimmons for providing us with the lightcurves shown in Fig. 1c. A. Fitzsimmons' careful review of the paper is greatly appreciated. The 4.2-m William Herschel Telescope is operated on the island of La Palma by the Royal Greenwich Observatory in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias. This research was performed at NASA/Jet Propulsion Laboratory, California Institute of Technology. JLO, FM and AM were supported by the Comision Nacional de Ciencia y Tecnologia under contracts ESP94-0719, ESP94-083, and ESP93-0338. GO and PYF were supported by the NASA Planetary Atmospheres Program.

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© European Southern Observatory (ESO) 1997

Online publication: May 26, 1998

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