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dc.contributor.author Belskaya, I. N.
dc.contributor.author Fornasier, S.
dc.contributor.author Tozzi, G. P.
dc.contributor.author Gil Hutton, Ricardo Alfredo
dc.contributor.author Cellino, A.
dc.contributor.author Antonyuk, K.
dc.contributor.author Krugly, Yu. N.
dc.contributor.author Dovgopol, A. N.
dc.contributor.author Faggi, S.
dc.date.available 2018-11-05T16:21:24Z
dc.date.issued 2017-03
dc.identifier.citation Belskaya, I. N.; Fornasier, S.; Tozzi, G. P.; Gil Hutton, Ricardo Alfredo; Cellino, A.; et al.; Refining the asteroid taxonomy by polarimetric observations; Academic Press Inc Elsevier Science; Icarus; 284; 3-2017; 30-42
dc.identifier.issn 0019-1035
dc.identifier.uri http://hdl.handle.net/11336/63617
dc.description.abstract We present new results of polarimetric observations of 15 main belt asteroids of different composition. By merging new and published data we determined polarimetric parameters characterizing individual asteroids and mean values of the same parameters characterizing different taxonomic classes. The majority of asteroids show polarimetric phase curves close to the average curve of the corresponding class. We show that using polarimetric data it is possible to refine asteroid taxonomy and derive a polarimetric classification for 283 main belt asteroids. Polarimetric observations of asteroid (21) Lutetia are found to exhibit possible variations of the position angle of the polarization plane over the surface.
dc.format application/pdf
dc.language.iso eng
dc.publisher Academic Press Inc Elsevier Science
dc.rights info:eu-repo/semantics/restrictedAccess
dc.rights.uri https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.subject ASTEROIDS
dc.subject COMPOSITION
dc.subject POLARIMETRY
dc.subject REGOLITHS
dc.subject.classification Astronomía
dc.subject.classification Ciencias Físicas
dc.subject.classification CIENCIAS NATURALES Y EXACTAS
dc.title Refining the asteroid taxonomy by polarimetric observations
dc.type info:eu-repo/semantics/article
dc.type info:ar-repo/semantics/artículo
dc.type info:eu-repo/semantics/publishedVersion
dc.date.updated 2018-10-22T17:24:57Z
dc.journal.volume 284
dc.journal.pagination 30-42
dc.journal.pais Países Bajos
dc.journal.ciudad Amsterdam
dc.description.fil Fil: Belskaya, I. N.. Karazin Kharkiv National University; Ucrania
dc.description.fil Fil: Fornasier, S.. Sorbonne Universités; Francia
dc.description.fil Fil: Tozzi, G. P.. Astrofisico di Arcetri; Italia
dc.description.fil Fil: Gil Hutton, Ricardo Alfredo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina. Universidad Nacional de San Juan; Argentina
dc.description.fil Fil: Cellino, A.. Astrofisico di Torino; Italia
dc.description.fil Fil: Antonyuk, K.. Crimean Astrophysical Observatory; Rusia
dc.description.fil Fil: Krugly, Yu. N.. Karazin Kharkiv National University; Ucrania
dc.description.fil Fil: Dovgopol, A. N.. Karazin Kharkiv National University; Ucrania
dc.description.fil Fil: Faggi, S.. Astrofisico di Arcetri; Italia
dc.journal.title Icarus
dc.relation.alternativeid info:eu-repo/semantics/altIdentifier/doi/https://dx.doi.org/10.1016/j.icarus.2016.11.003
dc.relation.alternativeid info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S0019103516302032
dc.conicet.fuente individual


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info:eu-repo/semantics/restrictedAccess Excepto donde se diga explícitamente, este item se publica bajo la siguiente descripción: Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Unported (CC BY-NC-SA 2.5)