Number of the records: 1  

Spin states of asteroids in the Eos collisional family

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    0494953 - ASÚ 2019 RIV US eng J - Journal Article
    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. … Total 37 authors
    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 - others:GA ČR(CZ) GA15-04816S
    Institutional support: RVO:67985815
    Keywords : main-belt asteroids * lightcurve inversion * photometric data
    OECD category: Astronomy (including astrophysics,space science)
    Impact factor: 3.565, year: 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.
    Permanent Link: http://hdl.handle.net/11104/0288006

     
     
Number of the records: 1  

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