Abstract. Photometric observations for 52 Europa (1995, 1999, 2000), 115 Thyra (1995, 1996, 2000, and 382 Dodona (1996, 1998, 1999, 2001) carried out at seven observatories are presented. Using all available lightcurves, the spin vectors, senses of rotation, and shape models of these three asteroids have been determined or refined.
out at six observatories are presented. Using all available lightcurves, the spin vectors, senses of rotation and shape models of these three asteroids were determined.
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