http://arxiv.org/abs/1906.01064
The main aim of photometrical observations of the asteroid 3200 Phaethon was searching for its low-level cometary activity (possible coma and/or dust tail) in the pre-perihelion passage. We performed observational runs with telescopes ranging from 0.61-m to 2-m and BVR color imaging. Three longer photometric series were used for modeling of the 3D shape of Phaethon. The color indices and size of the asteroid were estimated.
A. Kartashova, M. Husarik, O. Ivanova, et. al.
Wed, 5 Jun 19
55/74
Comments: 6 pages, 2 figures, 1 table