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Analysis of the rotation period of asteroids (1865) Cerberus, (2100) Ra-Shalom, and (3103) Eger – search for the YORP effect
- 1.0388185 - ASÚ 2013 RIV FR eng J - Journal Article
Ďurech, J. - Vokrouhlický, D. - Baransky, A.R. - Breiter, S. - Burkhonov, O.A. - Cooney, W.R. - Fuller, V. - Gaftonyuk, N. M. - Gross, J. - Inasaridze, R.Ya. - Kaasalainen, M. - Krugly, Yu. N. - Kvaratshelia, O.I. - Litvinenko, E.A. - Macomber, B. - Marchis, F. - Molotov, I.E. - Oey, J. - Polishook, D. - Pollock, J. - Pravec, Petr - Sárneczky, K. - Shevchenko, V. G. - Slyusarev, I. - Stephens, R. - Szabó, G. - Terrell, D. - Vachier, F. - Vanderplate, Z. - Viikinkoski, M. - Warner, B. D.
Analysis of the rotation period of asteroids (1865) Cerberus, (2100) Ra-Shalom, and (3103) Eger – search for the YORP effect.
Astronomy & Astrophysics. Roč. 547, November (2012), A10/1-A10/9. ISSN 0004-6361. E-ISSN 1432-0746
R&D Projects: GA ČR GAP209/12/0229
Institutional support: RVO:67985815
Keywords : minor planets * asteroids * data analysis
Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
Impact factor: 5.084, year: 2012
We analyzed photometric lightcurves of near-Earth asteroids (1865) Cerberus, (2100) Ra-Shalom, and (3103) Eger with the aim to detect possible deviations from the constant rotation caused by the YORP effect.
Permanent Link: http://hdl.handle.net/11104/0217015
Number of the records: 1