Romania / United States / Canada / Australia / Portugal / Slovakia / United Kingdom / Ukraine / Spain / Czech Republic / /
Currency
pence / / /
Facility
Italy Capote Observatory / Science Observatory / Research Institute / Charles University / Ukraine Institute of Applied Mathematics / Bonn University / Paint Trail / Modra Hill Observatory / University of Western Ontario / Catino Observatory / Sonoita Institute / SETI Institute / Elginfield Observatory / Carl Astronomical Observatory / Palmer Institute / University of California at Berkeley / Germany Divide Observatory / Palmer Divide Observatory / University of Warwick / U.S.A. Hill Observatory / Australia Observatory / University of North Carolina / Shed Observatory / Institute Institute / Appalachian State University / Chapel Hill / Crimean Astrophysical Observatory / University of North Dakota / Slovakia Research Observatory / Institute of Astronomy / Kharkiv National University / U.S.A. Observatory / / /
IndustryTerm
close asteroid binary systems / orbit solution / asteroids / close systems / main-belt binary systems / web page http /
Organization
University of California / University of North Dakota / Grand Forks / Palmer Institute for Astronomy / AS CR / Institute Institute / Academy of Sciences / SETI Institute / Kharkiv National University / Sonoita Institute / Simeiz Department / Ukraine Institute of Applied Mathematics / Department of Physics / Slovak Academy of Sciences / Instituto Politecnico de Tomar / Department of Astronomy / Research Institute / Bonn University / Charles University / Prague / Appalachian State University / Institute of Astronomy / University of Western Ontario / London / Faculty of Physics / University of North Carolina / Chapel Hill / Physics and Astronomy Department / Astronomy Department / University of Warwick / Academy of Sciences of the Czech Republic / Russia Sagan Center / /
Person
Petr Pravec / / /
ProvinceOrState
Minnesota / North Dakota / South Dakota / North Carolina / California / Arizona / Colorado / Ontario / /
Binary Asteroid Population. 2. Anisotropic distribution of orbit poles P. Pravec a, P. Scheirich a, D. Vokrouhlick´y b, A. W. Harris c, P. Kuˇsnir´ak a, K. Hornoch a, D. P. Pray d, D. Higgins e, ˇ Gajdoˇs f , L. Kor