Publicação: 2060 Chiron back to a minimum of brightness
dc.contributor.author | Lazzaro, D. | |
dc.contributor.author | Florczak, M. A. | |
dc.contributor.author | Betzler, A. | |
dc.contributor.author | Winter, O. C. | |
dc.contributor.author | GiuliattiWinter, S. M. | |
dc.contributor.author | Angeli, C. A. | |
dc.contributor.author | Foryta, D. W. | |
dc.contributor.institution | Centro Federal de Educação Tecnológica (CEFET) | |
dc.contributor.institution | Universidade Estadual Paulista (Unesp) | |
dc.contributor.institution | OBSERV PARIS | |
dc.contributor.institution | Universidade Federal do Paraná (UFPR) | |
dc.contributor.institution | Universidade Federal do Rio de Janeiro (UFRJ) | |
dc.date.accessioned | 2014-05-20T15:20:12Z | |
dc.date.available | 2014-05-20T15:20:12Z | |
dc.date.issued | 1996-12-01 | |
dc.description.abstract | The results of photometric observations of comet/steroid 2060 Chiron at the Observatorio do Pico dos Dias (Brazil - OPD) and the Observatoire de Haute-Provence (France - OHP) during 1994 and 1995 are presented. The analysis of the data shows a decrease of 2060. Chiron brightness from its peak values of 1988-1991. The absolute magnitude, H-V, varies from a maximum of 6.6 in February 1994 up to a minimum of 6.8 in June 1995. Therefore 2060 Chiron is back to a minimum of activity close to that of 1983-1985. The slope parameter G is found to be G = 0.71 +/- 0.15. It is suggested that the H-G magnitude system, generally adopted to present 2060 Chiron brightness, is not the most appropriate due to the cometary activity of this object. Copyright (C) 1996 Elsevier B.V. Ltd. | en |
dc.description.affiliation | CEFET,DEPT FIS,BR-80000 CURITIBA,PARANA,BRAZIL | |
dc.description.affiliation | UNESP,GRP DINAM ORBITAL & PLANETOL,GUARATINGUETA,BRAZIL | |
dc.description.affiliation | OBSERV PARIS,EUROPA,F-92195 MEUDON,FRANCE | |
dc.description.affiliation | UNIV FED PARANA,DEPT FIS,BR-80000 CURITIBA,PARANA,BRAZIL | |
dc.description.affiliation | FED UNIV RIO DE JANEIRO,OBS VALONGO,RIO JANEIRO,BRAZIL | |
dc.description.affiliationUnesp | UNESP,GRP DINAM ORBITAL & PLANETOL,GUARATINGUETA,BRAZIL | |
dc.format.extent | 1547-1550 | |
dc.identifier | http://dx.doi.org/10.1016/S0032-0633(96)00111-0 | |
dc.identifier.citation | Planetary and Space Science. Oxford: Pergamon-Elsevier B.V., v. 44, n. 12, p. 1547-1550, 1996. | |
dc.identifier.doi | 10.1016/S0032-0633(96)00111-0 | |
dc.identifier.issn | 0032-0633 | |
dc.identifier.lattes | 0960024575647258 | |
dc.identifier.uri | http://hdl.handle.net/11449/31547 | |
dc.identifier.wos | WOS:A1996WX73500003 | |
dc.language.iso | eng | |
dc.publisher | Elsevier B.V. | |
dc.relation.ispartof | Planetary and Space Science | |
dc.relation.ispartofjcr | 1.820 | |
dc.relation.ispartofsjr | 1,065 | |
dc.rights.accessRights | Acesso restrito | |
dc.source | Web of Science | |
dc.title | 2060 Chiron back to a minimum of brightness | en |
dc.type | Artigo | |
dcterms.license | http://www.elsevier.com/about/open-access/open-access-policies/article-posting-policy | |
dcterms.rightsHolder | Elsevier B.V. | |
dspace.entity.type | Publication | |
unesp.author.lattes | 0960024575647258 | |
unesp.campus | Universidade Estadual Paulista (UNESP), Faculdade de Engenharia, Guaratinguetá | pt |
unesp.department | Matemática - FEG | pt |
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