Physical models of ten asteroids from an observers' collaboration network

被引：22
|
作者：
Durech, J.
Kaasalainen, M.
Marciniak, A.
Allen, W. H.
Behrend, R.
Bembrick, C.
Bennett, T.
Bernasconi, L.
Berthier, J.
Bolt, G.
Boroumand, S.
da Silva, L. Crespo
Crippa, R.
Crow, M.
Durkee, R.
Dymock, R.
Fagas, M.
Fauerbach, M.
Fauvaud, S.
Frey, M.
Goncalves, R.
Hirsch, R.
Jardine, D.
Kamimski, K.
Koff, R.
Kwiatkowski, T.
Lopez, A.
Manzini, F.
Michalowski, T.
Pacheco, R.
Pan, M.
Pilcher, F.
Poncy, R.
Pray, D.
Pych, W.
Roy, R.
Santacana, G.
Slivan, S.
Sposetti, S.
Stephens, R.
Warner, B.
Wolf, M.
机构：
[1] Charles Univ Prague, Inst Astron, CR-18000 Prague, Czech Republic
[2] Univ Helsinki, Rolf Nevanlinna Inst, Dept Math & Stat, FIN-00014 Helsinki, Finland
[3] Adam Mickiewicz Univ Poznan, Astron Observ, PL-60286 Poznan, Poland
来源：
ASTRONOMY & ASTROPHYSICS | 2007年 / 465卷 / 01期
关键词：
minor planets; asteroids;
D O I：
10.1051/0004-6361:20066347
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Aims. We present physical models of ten asteroids obtained by means of lightcurve inversion. A substantial part of the photometric data was observed by amateur astronomers. We emphasize the importance of a coordinated network of observers that will be of extreme importance for future all-sky asteroid photometric surveys. Methods. The lightcurve inversion method was used to derive spin states and shape models of the asteroids. Results. We derived spin states and shape model for ten new asteroids: (110) Lydia, (125) Liberatrix, (130) Elektra, (165) Loreley, (196) Philomela, (218) Bianca, (306) Unitas, (423) Diotima, (776) Berbericia, and (944) Hidalgo. This increases the number of asteroid models up to nearly one hundred.
引用
收藏
页码：331 / U64
页数：12
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