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dc.contributor.author
Sokova, Iraida A.
dc.contributor.author
Sokov, Eugenii N.
dc.contributor.author
Gorshanov, Denis L.
dc.contributor.author
Fernandez Lajus, Eduardo Eusebio
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Di Sisto, Romina Paula
dc.contributor.author
Bretton, Marc
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Marchini, Alessandro
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Vasilkova, Olga O.
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Knight, Carl R.
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Colazo, Carlos Roberto
dc.contributor.author
Quiñones, Cecilia
dc.contributor.author
Girardini, Carla
dc.date.available
2021-02-12T19:31:25Z
dc.date.issued
2019-05
dc.identifier.citation
Sokova, Iraida A.; Sokov, Eugenii N.; Gorshanov, Denis L.; Fernandez Lajus, Eduardo Eusebio; Di Sisto, Romina Paula; et al.; Results of the investigation of the asteroid (2121) Sevastopol based on photometric observations of mutual phenomena; Pergamon-Elsevier Science Ltd; Planetary and Space Science; 175; 5-2019; 25-33
dc.identifier.issn
0032-0633
dc.identifier.uri
http://hdl.handle.net/11336/125639
dc.description.abstract
The asteroid (2121) Sevastopol is a binary asteroid from the main belt. The duplicity of the asteroid was discovered based on photometric observations of mutual phenomena (eclipses and occultations) that were detected in its light curves (Higgins et al., 2010). We organized a photometrical observational campaign for the observations of mutual phenomena in binary system of the asteroid (2121) Sevastopol and an investigation of the properties of the asteroid's satellite. The observations allowed us to define mass, density, taxonomical class and preliminary orbit of the satellite of the asteroid (2121) Sevastopol.
dc.format
application/pdf
dc.language.iso
eng
dc.publisher
Pergamon-Elsevier Science Ltd
dc.rights
info:eu-repo/semantics/restrictedAccess
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.subject
ASTEROIDS
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ASTEROIDS
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CELESTIAL MECHANICS
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DYNAMICS
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ROTATION
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SATELLITES OF ASTEROIDS
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Astronomía
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Ciencias Físicas
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CIENCIAS NATURALES Y EXACTAS
dc.title
Results of the investigation of the asteroid (2121) Sevastopol based on photometric observations of mutual phenomena
dc.type
info:eu-repo/semantics/article
dc.type
info:ar-repo/semantics/artículo
dc.type
info:eu-repo/semantics/publishedVersion
dc.date.updated
2020-11-19T22:01:53Z
dc.journal.volume
175
dc.journal.pagination
25-33
dc.journal.pais
Estados Unidos
dc.journal.ciudad
Amsterdam
dc.description.fil
Fil: Sokova, Iraida A.. Pulkovo Observatory; Rusia
dc.description.fil
Fil: Sokov, Eugenii N.. Pulkovo Observatory; Rusia. Special Astrophysical Observatory ; Rusia
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Fil: Gorshanov, Denis L.. Pulkovo Observatory; Rusia
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Fil: Fernandez Lajus, Eduardo Eusebio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
dc.description.fil
Fil: Di Sisto, Romina Paula. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
dc.description.fil
Fil: Bretton, Marc. Baronnies Provençales Observatory; Francia
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Fil: Marchini, Alessandro. Università degli Studi di Siena; Italia
dc.description.fil
Fil: Vasilkova, Olga O.. Pulkovo Observatory; Rusia
dc.description.fil
Fil: Knight, Carl R.. Ngileah Observatory; Nueva Zelanda
dc.description.fil
Fil: Colazo, Carlos Roberto. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina
dc.description.fil
Fil: Quiñones, Cecilia. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina
dc.description.fil
Fil: Girardini, Carla. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina
dc.journal.title
Planetary and Space Science
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://linkinghub.elsevier.com/retrieve/pii/S003206331830415X
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1016/j.pss.2019.05.007
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