Asteroid (216) Kleopatra

Tests of the radar-derived shape model

D. Hestroffer¹ - J. Berthier¹ - P. Descamps¹ - P. Tanga^2, - A. Cellino² - M. Lattanzi² - M. Di Martino² - V. Zappalà²

1 - IMCCE, UMR CNRS 8028, Observatoire de Paris, 77 Av. Denfert Rochereau, 75014 Paris, France
2 - Osservatorio Astronomico di Torino (OATo), Strada Osservatorio 20, 10025 Pino Torinese (TO), Italy

A&A, 392, 729-733 (2002), DOI: 10.1051/0004-6361:20021006

Figure 1 has been misprinted so we print it again.

$\begin{figure} \centering \resizebox{\hsize}{!}{ \includegraphics{H3771f1New.eps} \includegraphics{H3771f2New.eps} }\end{figure}$	Figure 1: Comparison between the observed occultation data and the radar model. Left panel: occultation of Oct. 10, 1980 at 7.00h UTC. Right panel: occultation of Jan. 1, 1991 at 5.28h UTC. The dashed lines correspond to negative observations. Error bars are given by crosses and are negligible for the photoelectric observations.
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