Photometry and models of selected main belt asteroids -: I.: 52 Europa, 115 Thyra, and 382 Dodona

被引：27
|
作者：
Michalowski, T
Kwiatkowski, T
Kaasalainen, M
Pych, W
Kryszczynska, A
Dybczynski, PA
Velichko, FP
Erikson, A
Denchev, P
Fauvaud, S
Szabó, GM
机构：
[1] Adam Mickiewicz Univ, Astron Observ, PL-60286 Poznan, Poland
[2] Univ Helsinki, Rolf Nevanlinna Inst, FIN-00014 Helsinki, Finland
[3] Copernicus Astron Ctr, PL-00716 Warsaw, Poland
[4] Kharkiv Karazin Natl Univ, Res Inst Astron, UA-61022 Kharkov, Ukraine
[5] Inst Space Sensor Technol & Planetary Explorat, D-12489 Berlin, Germany
[6] Rozhen Natl Observ, Inst Astron, Smoljan 4700, Bulgaria
[7] Astroqueyras Assoc, F-05350 Mairie, St Veran, France
[8] Univ Szeged, Dept Expt Phys, H-6720 Szeged, Hungary
[9] Univ Szeged, Astron Observ, H-6720 Szeged, Hungary
[10] Isaac Newton Inst Chile, Crimean Branch, Nauchnyi, Ukraine
来源：
ASTRONOMY & ASTROPHYSICS | 2004年 / 416卷 / 01期
关键词：
techniques : photometric; minor planets; asteroids;
D O I：
10.1051/0004-6361:20031706
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Photometric observations for 52 Europa (1995, 1997, 1999, 2000), 115 Thyra (1995, 1996, 1998, 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.
引用
收藏
页码：353 / 366
页数：14
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