New photometric observations of asteroids (1862) Apollo and (25143) Itokawa - An analysis of YORP effect

Astronomy and Astrophysics

Volumn 488, Issue 1, 2008, Pages 345-350

  Durech J ^a   Vokrouhlicky D ^a   Kaasalainen, M ^b   Weissman, P ^c   Lowry, S C ^c   Beshore, E ^d   Higgins, D ^e   Krugly, Y N ^f   Shevchenko, V G ^f   Gaftonyuk, N M ^g   Choi, Y J ^c,h   Kowalski, R A ^d   Larson, S ^d   Warner, B D ⁱ   Marshalkina, A L ^j   Ibrahimov, M A ^j   Molotov, I E ^k   Michalowski T ^l   Kitazato, K ^m  

^a CHARLES UNIVERSITY   (Czech Republic)

^b UNIVERSITY OF HELSINKI   (Finland)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^d UNIVERSITY OF ARIZONA   (United States)

^e Hunters Hill Observatory   (Australia)

^f V N KARAZIN KHARKIV NATIONAL UNIVERSITY   (Ukraine)

^g CRIMEAN ASTROPHYSICAL OBSERVATORY   (Ukraine)

^h Korea Astronomy and Space Science Institute (KASI)   (South Korea)

ⁱ Palmer Divide Observatory   (United States)

^j S YU YUNUSOV INSTITUTE OF THE CHEMISTRY OF PLANT SUBSTANCES   (Uzbekistan)

^k KELDYSH INSTITUTE OF APPLIED MATHEMATICS   (Russian Federation)

^l ADAM MICKIEWICZ UNIVERSITY   (Poland)

^m UNIVERSITY OF TOKYO   (Japan)

more..

Author keywords

Methods: data analysis; Minor planets, asteroids; Techniques: photometric

Indexed keywords

FORECASTING; METAL WORKING SHAPERS; PHOTOMETRY; ROTATION; SPIN DYNAMICS;

FREE PARAMETERS; HIGH DEGREE OF ACCURACY; INVERSION METHODS; ITOKAWA; METHODS: DATA ANALYSIS; MINOR PLANETS, ASTEROIDS; NEW MODEL; ROTATION PERIODS; ROTATION RATES; SHAPE MODELLING; SPIN STATES; TECHNIQUES: PHOTOMETRIC; TIME-LINE; UPPER LIMITS;

ASTEROIDS;

EID: 49749129246     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809663     Document Type: Article

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