CCD photometry, spin and shape models of five asteroids: 225, 360, 416, 516, and 1223

Details CCD photometry, spin and shape models of five asteroids: 225, 360, 416, 516, and 1223 CCD photometry, spin and shape models of five asteroids: 225, 360, 416, 516, and 1223

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000a%26as..146..471m&link_type=abstract

Astronomy and Astrophysics Supplement, v.146, p.471-479

Astronomy and Astrophysics

Astrophysics

12

Techniques: Photometric, Minor Planets: Asteroids

Scientific paper

New CCD photometric observations for 225 Henrietta (1995), 360 Carlova (1996, 1997, 1998), 416 Vaticana (1995-96, 1998), 516 Amherstia (1995, 1996), and 1223 Neckar (1995-96) carried out at five observatories are presented. New synodical periods for two asteroids (225, 1223) have been obtained. Using all available lightcurves, the spin vectors, senses of rotation, and triaxial elipsoid models of these five asteroids have been determined or refined.

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