Abstract
Results of observations of small (less than 140 m in diameter) near-Earth asteroids (NEAs) and observations of NEAs at a low solar elongation are presented. All of the results were obtained in the Research Institute Nikolaev Astronomical Observatory with the combined method of observations and the “time delay and integration” operation mode of the CCD camera.
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Original Russian Text © V.S. Vovk, N.A. Kulichenko, E.S. Kozyryev, E.S. Sybiryakova, O.V. Shulga, 2015, published in Kinematika i Fizika Nebesnykh Tel, 2015, Vol. 31, No. 3, pp. 73–80.
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Vovk, V.S., Kulichenko, N.A., Kozyryev, E.S. et al. Observations of near-Earth asteroids of small sizes and at a low solar elongation. Kinemat. Phys. Celest. Bodies 31, 154–159 (2015). https://doi.org/10.3103/S0884591315030071
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DOI: https://doi.org/10.3103/S0884591315030071