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Volumn 316, Issue 5822, 2007, Pages 272-274

Direct detection of the asteroidal YORP effect

Author keywords

[No Author keywords available]

Indexed keywords

ASTEROID; DETECTION METHOD; PHOTOMETER; PLANETARY ROTATION; SOLAR SYSTEM;

EID: 34247358673     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1139040     Document Type: Article
Times cited : (179)

References (17)
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    • W. F. Bottke, A. Cellino, P. Paolicchi, R. Binzel, Eds, Univ. of Arizona Press, Tucson, AZ
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    • (2002) Asteroids III , pp. 113-122
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    • W. F. Bottke, D. Vokrouhlický, D. P. Rubincam, M. Broz, in Asteroids III, W. F. Bottke, A. Cellino, P. Paolicchi, R. Binzel, Eds. (Univ. of Arizona Press, Tucson, AZ, 2002), pp. 395-408.
    • (2002) Asteroids III , pp. 395-408
    • Bottke, W.F.1    Vokrouhlický, D.2    Rubincam, D.P.3    Broz, M.4
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    • P. A. Taylor et al., Science 316, 274 (2007); published online 8 March 2007 (10.1126/science.1139038).
    • P. A. Taylor et al., Science 316, 274 (2007); published online 8 March 2007 (10.1126/science.1139038).
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    • See supporting material on Science Online.
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    • We thank all the staff at the observatories involved in this study for their support. This work was based on observations at the following observatories: ESO, Chile (PIDs 271.C-5023 and 073.C-0137, Ondrejov Observatory, Czech Republic (grant A3003204, Centro Astronómico Hispano Atemán (Calar Alto, Spain, Liverpool Telescope, La Palma (Canary Islands, Spain, Isaac Newton Group, La Patma; and Faulkes Telescope North (Maui, Hawaii, We also thank the referees for their helpful reviews. Supported by the Leverhulme Trust (S.C.L, the UK Particle Physics and Astronomy Research Council (A.F, the Grant Agency of the Czech Republic (P.P. and D.V, NASA grant NNG04GN31G (P.A.T. and J.-L.M, and Slovak Grant Agency for Science VEGA grant 1/3074/06 A.G, This work made use of the NASA/JPL HORIZONS ephemeris-generating program
    • We thank all the staff at the observatories involved in this study for their support. This work was based on observations at the following observatories: ESO, Chile (PIDs 271.C-5023 and 073.C-0137); Ondrejov Observatory, Czech Republic (grant A3003204); Centro Astronómico Hispano Atemán (Calar Alto, Spain); Liverpool Telescope, La Palma (Canary Islands, Spain); Isaac Newton Group, La Patma; and Faulkes Telescope North (Maui, Hawaii). We also thank the referees for their helpful reviews. Supported by the Leverhulme Trust (S.C.L.), the UK Particle Physics and Astronomy Research Council (A.F.), the Grant Agency of the Czech Republic (P.P. and D.V.), NASA grant NNG04GN31G (P.A.T. and J.-L.M.), and Slovak Grant Agency for Science VEGA grant 1/3074/06 (A.G.). This work made use of the NASA/JPL HORIZONS ephemeris-generating program.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.