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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
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Ciencias Físicas
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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


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