Publicação:
2060 Chiron back to a minimum of brightness

dc.contributor.authorLazzaro, D.
dc.contributor.authorFlorczak, M. A.
dc.contributor.authorBetzler, A.
dc.contributor.authorWinter, O. C.
dc.contributor.authorGiuliattiWinter, S. M.
dc.contributor.authorAngeli, C. A.
dc.contributor.authorForyta, D. W.
dc.contributor.institutionCentro Federal de Educação Tecnológica (CEFET)
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.contributor.institutionOBSERV PARIS
dc.contributor.institutionUniversidade Federal do Paraná (UFPR)
dc.contributor.institutionUniversidade Federal do Rio de Janeiro (UFRJ)
dc.date.accessioned2014-05-20T15:20:12Z
dc.date.available2014-05-20T15:20:12Z
dc.date.issued1996-12-01
dc.description.abstractThe 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.affiliationCEFET,DEPT FIS,BR-80000 CURITIBA,PARANA,BRAZIL
dc.description.affiliationUNESP,GRP DINAM ORBITAL & PLANETOL,GUARATINGUETA,BRAZIL
dc.description.affiliationOBSERV PARIS,EUROPA,F-92195 MEUDON,FRANCE
dc.description.affiliationUNIV FED PARANA,DEPT FIS,BR-80000 CURITIBA,PARANA,BRAZIL
dc.description.affiliationFED UNIV RIO DE JANEIRO,OBS VALONGO,RIO JANEIRO,BRAZIL
dc.description.affiliationUnespUNESP,GRP DINAM ORBITAL & PLANETOL,GUARATINGUETA,BRAZIL
dc.format.extent1547-1550
dc.identifierhttp://dx.doi.org/10.1016/S0032-0633(96)00111-0
dc.identifier.citationPlanetary and Space Science. Oxford: Pergamon-Elsevier B.V., v. 44, n. 12, p. 1547-1550, 1996.
dc.identifier.doi10.1016/S0032-0633(96)00111-0
dc.identifier.issn0032-0633
dc.identifier.lattes0960024575647258
dc.identifier.urihttp://hdl.handle.net/11449/31547
dc.identifier.wosWOS:A1996WX73500003
dc.language.isoeng
dc.publisherElsevier B.V.
dc.relation.ispartofPlanetary and Space Science
dc.relation.ispartofjcr1.820
dc.relation.ispartofsjr1,065
dc.rights.accessRightsAcesso restrito
dc.sourceWeb of Science
dc.title2060 Chiron back to a minimum of brightnessen
dc.typeArtigo
dcterms.licensehttp://www.elsevier.com/about/open-access/open-access-policies/article-posting-policy
dcterms.rightsHolderElsevier B.V.
dspace.entity.typePublication
unesp.author.lattes0960024575647258
unesp.campusUniversidade Estadual Paulista (UNESP), Faculdade de Engenharia, Guaratinguetápt
unesp.departmentMatemática - FEGpt

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