Work

Asteroid models from the Lowell photometric database

Year: 2016

Type: article

Abstract: Context. Information about shapes and spin states of individual asteroids is important for the study of the whole asteroid population. For asteroids from the main belt, most of the shape models available now have been reconstructed from disk-integrated photometry by the lightcurve inversion method.

Source: Astronomy and Astrophysics

DOI: 10.1051/0004-6361/201527573

Authors: J. Ďurech, J. Hanuš, D. Oszkiewicz, R. Vančo

Institutions: Charles University, Centre National de la Recherche Scientifique, Université Côte d'Azur, Centre National d'Études Spatiales, Lagrange Laboratory, Observatoire de la Côte d’Azur, Adam Mickiewicz University in Poznań

Language: English

Topic: Astro and Planetary Science

Subfield: Astronomy and Astrophysics

Field: Physics and Astronomy

Domain: Physical Sciences

Open Access status: bronze

Funders: Agence Nationale de la Recherche, Grantová Agentura České Republiky, Centre National d’Etudes Spatiales, Narodowe Centrum Nauki

Awards: A big picture of the main asteroid belt - physical properties of asteroids derived by inversion of optical and infrared photometry, G5627150172, G8589016346

OpenAlex ID: W2284980433

FWCI: 3.744

Cites: 26

Cited by: 59

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