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
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DOI：
10.1051/aas:2000282
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发表时间：
2000-11
期刊：
影响因子：
--
通讯作者：
T. Michałowski;W. Pych;J. Berthier;A. Kryszczyńska;T. Kwiatkowski;J. Boussuge;S. Fauvaud;P. Denchev;R. Baranowski
中科院分区：
文献类型：
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作者：
T. Michałowski;W. Pych;J. Berthier;A. Kryszczyńska;T. Kwiatkowski;J. Boussuge;S. Fauvaud;P. Denchev;R. Baranowski
本文介绍了在VE天文台对225个Henrietta(1995)，360 Carlova(1996,1997,1998)，416个Vaticana(1995(96,1998)，516 Amherstia(1995,1996)和1223 Neckar(1995(96))进行的新的CCD测光观测结果。获得了两个星体(225,1223)的新合点周期。利用所有可用的光曲线，已经确定或重新确定了这些VE小行星的自旋矢量、自转感和三轴椭球体模型。
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 ve observa- tories are presented. New synodical periods for two as- teroids (225, 1223) have been obtained. Using all avail- able lightcurves, the spin vectors, senses of rotation, and triaxial elipsoid models of these ve asteroids have been determined or rened.