Spin states of asteroids in the Eos collisional family

0494953 - ASÚ 2019 RIV US eng J - Článek v odborném periodiku
Hanuš, J. - Delbo, M. - Ali-Lagoa, V. - Bolin, B. - Jedicke, R. - Ďurech, J. - Cibulková, H. - Pravec, Petr - Kušnirák, Peter - Behrend, R. - Marchis, F. - Antonini, G. - Arnold, L. - Audejean, M. - Bachschmidt, M. - Bernasconi, L. - Brunetto, L. - Casulli, S. - Dymock, R. - Esseiva, N. - Esteban, M. - Gerteis, O. - de Groot, H. - Gully, H. - Hamanowa, H. - Krafft, P. - Lehký, M. - Manzini, F. - Michelet, J. - Pilcher, F. - Morelle, E. - Oey, J. - Reignier, F. - Roy, R. - Salom, P. A. - Warner, B. D. … celkem 37 autorů
Spin states of asteroids in the Eos collisional family.
Icarus. Roč. 299, January (2018), s. 84-96. ISSN 0019-1035. E-ISSN 1090-2643
Grant ostatní: GA ČR(CZ) GA15-04816S
Institucionální podpora: RVO:67985815
Klíčová slova: main-belt asteroids * lightcurve inversion * photometric data
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 3.565, rok: 2018

We aim to increase the number of asteroid shape models and rotation states within the Eos collision family, as well as to revise previously published shape models from the literature. Such results can be used to constrain theoretical collisional and evolution models of the family, or to estimate other physical parameters by a thermophysical modeling of the thermal infrared data. We use all available disk-integrated optical data as input for the convex inversion method, and derive 3D shape models of asteroids together with their rotation periods and orientations of rotation axes. We present updated shape models for 15 asteroids and new shape model determinations for 16 asteroids. Together with the already published models from the publicly available DAMIT database, we compiled a sample of 56 Eos family members with known shape models that we used in our analysis of physical properties within the family.
Trvalý link: http://hdl.handle.net/11104/0288006