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

Authors
Michalowski, T Pych, W Berthier, J Kryszczynska, A Kwiatkowski, T Boussuge, J Fauvaud, S Denchev, P Baranowski, R
Citation
T. Michalowski et al., CCD photometry, spin and shape models of five asteroids: 225, 360, 416, 516, and 1223, ASTR AST SS, 146(3), 2000, pp. 471-479
Citations number
29
Categorie Soggetti
Space Sciences
Journal title
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES
ISSN journal
03650138 → ACNP
Volume
146
Issue
3
Year of publication
2000
Pages
471 - 479
Database
ISI
SICI code
0365-0138(200011)146:3<471:CPSASM>2.0.ZU;2-A
Abstract
New CCD photometric observations for 225 Henrietta (1995), 360 Carlova (199 6: 1997? 1998), 416 Vaticana (1995 96, 1996), 516 Amherstia (1995, 1996), a nd 1223 Neckar (1995-96) carried out at five observatories are presented. N ew synodical periods for two asteroids (225, 1223) have been obtained. Usin g all available lightcurves, the spin vectors, senses of rotation, and tria xial elipsoid models of these five asteroids have been determined or refine d.