We present the results of photometric observations of 12 asteroids, pe
rformed from 1985 through 1989 at the Astronomical Observatory of Tera
mo (Italy), Astronomical Observatory of Turin (Italy), and European So
uthern Observatory (ESO, La Silla, Chile). Using the EA pole determina
tion method described in G. De Angelis (Planet. Space Sci., 41, 285-29
0, 1993), we have obtained the first spin and shape solution of 85 Io
and 360 Carlova and an improvement of the previous determinations for
12 Victoria, 192 Nausikaa and 423 Diotima, for which we determined for
the first time the sidereal period and the sense of rotation. We have
checked the determinations obtained by other authors for the asteroid
s 3 June, 6 Hebe, 20 Massalia, 43 Ariadne, and 52 Europa, and suggeste
d a very rough estimate of the spin and shape parameters of 115 Thyra.
(C) 1995 Academic Press, Inc.