Por favor, use este identificador para citar o enlazar este ítem: https://hdl.handle.net/20.500.12008/54069
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dc.contributor.author Autor Martino, Silvia-
dc.contributor.author Autor Tancredi Machado, Gonzalo José-
dc.contributor.author Autor Banda-Huarca, M.-
dc.contributor.filiacion Filiación Martino Silvia, Universidad de la República (Uruguay). Facultad de Ciencias. Instituto de Física.-
dc.contributor.filiacion Filiación Tancredi Machado Gonzalo José, Universidad de la República (Uruguay). Facultad de Ciencias. Instituto de Física.-
dc.contributor.filiacion Filiación Banda-Huarca M.-
dc.date.accessioned Fecha ingreso 2026-03-24T15:08:24Z-
dc.date.available Fecha disponible 2026-03-24T15:08:24Z-
dc.date.issued Año de publicación 2025-
dc.description Descripción En este artículo participan más de cuarenta autores.es
dc.description.abstract Resumen Context: Transitional objects are minor bodies that share some characteristics with asteroids and others with comets. These objects include asteroids in cometary orbits (ACOs), which behave dynamically like comets, but lack observed activity, while activated asteroids (AAs) follow typical asteroidal orbits, but have shown dust ejections. Aims: The monitoring of a set of these objects carried out in 2015 and 2016 is continued using archival images from various observatories and new data from the IMPACTON telescope in Brazil. Methods: Two techniques were applied to detect activity: (i) surface brightness profiles were compared with those of field stars to identify widening, and (ii) the magnitudes reported in the Minor Planet Center, combined with our observations, were reduced and analyzed to identify abrupt brightness increases as a function of heliocentric distance. Results: We analyzed the surface brightness profiles of 133 ACOs and 7 AAs. To study the reduced magnitude, we obtained data from the 705 ACOs that were known at the time of the analysis. Together with the data from our previous work, our analysis covered 23% of the total known ACOs; 8 deviated slightly in the surface brightness profile, 6 brightened in the reduced magnitude, and one object is in common in both samples. A very low percentage of objects might show activity (4% of the sample with brightness profiles and <1% in the reduced magnitudes). These results would rule out a slow transition from active to inert. Regarding AAs, 4 showed activity, and 3 of them matched previously reported periods, while the data we analyzed for P/2015 X6 were obtained 19 days before the first existing activity report. The activity episodes of these objects are very restricted in time and do not always occur in the same region of the orbit.es
dc.description.sponsorship Financiadores CSIC: I+D_C630-348es
dc.description.sponsorship Financiadores CSIC: I+D_C630-347es
dc.format.extent Extensión 16 hes
dc.format.mimetype Formato application/pdfes
dc.identifier.citation Citación Martino, S, Tancredi Machado, G, Banda-Huarca, M [y otros autores]. "Monitoring of asteroids in cometary orbits and activated asteroids through archival images and new observations". Astronomy & Astrophysics. [en línea] 2025, 698: A117. 16 h. DOI: 10.1051/0004-6361/202554124es
dc.identifier.doi DOI 10.1051/0004-6361/202554124-
dc.identifier.issn ISSN 1432-0746-
dc.identifier.uri URI https://hdl.handle.net/20.500.12008/54069-
dc.language.iso Idioma enes
dc.publisher Editorial EDP Scienceses
dc.relation.ispartof EN Astronomy & Astrophysics, 2025, 698: A117.es
dc.rights Derechos Las obras depositadas en el Repositorio se rigen por la Ordenanza de los Derechos de la Propiedad Intelectual de la Universidad de la República.(Res. Nº 91 de C.D.C. de 8/III/1994 – D.O. 7/IV/1994) y por la Ordenanza del Repositorio Abierto de la Universidad de la República (Res. Nº 16 de C.D.C. de 07/10/2014)es
dc.rights.licence Licencia Licencia Creative Commons Atribución (CC - By 4.0)es
dc.subject Palabras clave Cometses
dc.subject Palabras clave Minor planetses
dc.subject Palabras clave Asteroidses
dc.title Título Monitoring of asteroids in cometary orbits and activated asteroids through archival images and new observationses
dc.type Tipo de documento Artículoes
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10.1051.0004-6361.202554124.pdf — 6.83 MB Adobe PDF