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dc.contributor.author
Morgado, B.E.  
dc.contributor.author
Sicardy, Bruno  
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Braga Ribas, Felipe  
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Desmars, Josselin  
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Gomes Júnior, Altair Ramos  
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Bérard, D.  
dc.contributor.author
Leiva, Rodrigo  
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Vieira Martins, Roberto  
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Benedetti Rossi, G.  
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Santos Sanz, Pablo  
dc.contributor.author
Camargo, Julio Ignacio Bueno  
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Duffard, R.  
dc.contributor.author
Rommel, F.L.  
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Assafin, M.  
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Boufleur, R.C.  
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Colas, F.  
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Kretlow, Mike  
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Beisker, W.  
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Sfair, Rafael  
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Snodgrass, Colin  
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Morales, N.  
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Fernández Valenzuela, E.  
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Amaral, L.S.  
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Amarante, A.  
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Artola, R.A.  
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Backes, M.  
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Bath, K. L.  
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Bouley, S.  
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Garcia Lambas, Diego Rodolfo  
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Schneiter, Ernesto Matías  
dc.date.available
2022-10-13T15:46:49Z  
dc.date.issued
2021-08  
dc.identifier.citation
Morgado, B.E.; Sicardy, Bruno; Braga Ribas, Felipe; Desmars, Josselin; Gomes Júnior, Altair Ramos; et al.; Refined physical parameters for Chariklo's body and rings from stellar occultations observed between 2013 and 2020; EDP Sciences; Astronomy and Astrophysics; 652; A141; 8-2021; 1-29  
dc.identifier.issn
0004-6361  
dc.identifier.uri
http://hdl.handle.net/11336/173040  
dc.description.abstract
Context. The Centaur (10199) Chariklo has the first ring system discovered around a small object. It was first observed using stellar occultation in 2013. Stellar occultations allow sizes and shapes to be determined with kilometre accuracy, and provide the characteristics of the occulting object and its vicinity. Aims. Using stellar occultations observed between 2017 and 2020, our aim is to constrain the physical parameters of Chariklo and its rings. We also determine the structure of the rings, and obtain precise astrometrical positions of Chariklo. Methods. We predicted and organised several observational campaigns of stellar occultations by Chariklo. Occultation light curves were measured from the datasets, from which ingress and egress times, and the ring widths and opacity values were obtained. These measurements, combined with results from previous works, allow us to obtain significant constraints on Chariklo's shape and ring structure. Results. We characterise Chariklo's ring system (C1R and C2R), and obtain radii and pole orientations that are consistent with, but more accurate than, results from previous occultations. We confirm the detection of W-shaped structures within C1R and an evident variation in radial width. The observed width ranges between 4.8 and 9.1 km with a mean value of 6.5 km. One dual observation (visible and red) does not reveal any differences in the C1R opacity profiles, indicating a ring particle size larger than a few microns. The C1R ring eccentricity is found to be smaller than 0.022 (3σ), and its width variations may indicate an eccentricity higher than ~0.005. We fit a tri-axial shape to Chariklo's detections over 11 occultations, and determine that Chariklo is consistent with an ellipsoid with semi-axes of 143.8-1.5+1.4, 135.2-2.8+1.4, and 99.1-2.7+5.4 km. Ultimately, we provided seven astrometric positions at a milliarcsecond accuracy level, based on Gaia EDR3, and use it to improve Chariklo's ephemeris.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
EDP Sciences  
dc.rights
info:eu-repo/semantics/openAccess  
dc.rights.uri
https://creativecommons.org/licenses/by/2.5/ar/  
dc.subject
ASTEROIDS: INDIVIDUAL: CHARIKLO  
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METHODS: DATA ANALYSIS  
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METHODS: OBSERVATIONAL  
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MINOR PLANETS  
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OCCULTATIONS  
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PLANETS AND SATELLITES: RINGS  
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Astronomía  
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Ciencias Físicas  
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CIENCIAS NATURALES Y EXACTAS  
dc.title
Refined physical parameters for Chariklo's body and rings from stellar occultations observed between 2013 and 2020  
dc.type
info:eu-repo/semantics/article  
dc.type
info:ar-repo/semantics/artículo  
dc.type
info:eu-repo/semantics/publishedVersion  
dc.date.updated
2022-09-21T13:53:15Z  
dc.identifier.eissn
1432-0746  
dc.journal.volume
652  
dc.journal.number
A141  
dc.journal.pagination
1-29  
dc.journal.pais
Francia  
dc.journal.ciudad
Paris  
dc.description.fil
Fil: Morgado, B.E.. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; Brasil  
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Fil: Sicardy, Bruno. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia  
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Fil: Braga Ribas, Felipe. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; Brasil. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia. Universidade Tecnologia Federal do Parana; Brasil  
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Fil: Desmars, Josselin. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia  
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Fil: Gomes Júnior, Altair Ramos. Universidade de Sao Paulo; Brasil  
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Fil: Bérard, D.. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia  
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Fil: Leiva, Rodrigo. Universidad de Chile; Chile. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia  
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Fil: Vieira Martins, Roberto. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; Brasil. Universidade Federal do Rio de Janeiro; Brasil  
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Fil: Benedetti Rossi, G.. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia. Universidade Federal de Sao Paulo; Brasil  
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Fil: Santos Sanz, Pablo. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; Brasil  
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Fil: Camargo, Julio Ignacio Bueno. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; Brasil  
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Fil: Duffard, R.. Universidade Federal do Rio de Janeiro; Brasil  
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Fil: Rommel, F.L.. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; Brasil  
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Fil: Assafin, M.. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia  
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Fil: Boufleur, R.C.. Universidad Nacional de Córdoba; Argentina  
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Fil: Colas, F.. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; Brasil  
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Fil: Kretlow, Mike. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; Brasil  
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Fil: Beisker, W.. University of North Carolina; Estados Unidos  
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Fil: Sfair, Rafael. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia  
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Fil: Snodgrass, Colin. University of Edinburgh; Reino Unido  
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Fil: Morales, N.. Pontificia Universidad Católica de Chile; Chile. Universidad Católica de Chile; Chile  
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Fil: Fernández Valenzuela, E.. Pontificia Universidad Católica de Chile; Chile. Universidad Católica de Chile; Chile  
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Fil: Amaral, L.S.. Massachusetts Institute of Technology; Estados Unidos  
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Fil: Amarante, A.. Ministério de Ciencia, Tecnologia e Innovacao. Observatorio Nacional; Brasil  
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Fil: Artola, R.A.. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia  
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Fil: Backes, M.. Universidad Nacional de Córdoba; Argentina  
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Fil: Bath, K. L.. University of North Carolina; Estados Unidos  
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Fil: Bouley, S.. University of St. Andrews; Reino Unido  
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Fil: Garcia Lambas, Diego Rodolfo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina  
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Fil: Schneiter, Ernesto Matías. Universidad Nacional de Córdoba. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Ingeniería Económica y Legal; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina  
dc.journal.title
Astronomy and Astrophysics  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1051/0004-6361/202141543  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/full_html/2021/08/aa41543-21/aa41543-21.html