2060 Chiron back to a minimum of brightness

dc.contributorUniversidade Estadual Paulista (UNESP)
dc.creatorLazzaro, D.
dc.creatorFlorczak, M. A.
dc.creatorBetzler, A.
dc.creatorWinter, O. C.
dc.creatorGiuliattiWinter, S. M.
dc.creatorAngeli, C. A.
dc.creatorForyta, D. W.
dc.date2014-05-20T15:20:12Z
dc.date2016-10-25T17:53:17Z
dc.date2014-05-20T15:20:12Z
dc.date2016-10-25T17:53:17Z
dc.date1996-12-01
dc.date.accessioned2017-04-05T23:24:36Z
dc.date.available2017-04-05T23:24:36Z
dc.identifierPlanetary and Space Science. Oxford: Pergamon-Elsevier B.V., v. 44, n. 12, p. 1547-1550, 1996.
dc.identifier0032-0633
dc.identifierhttp://hdl.handle.net/11449/31547
dc.identifierhttp://acervodigital.unesp.br/handle/11449/31547
dc.identifier10.1016/S0032-0633(96)00111-0
dc.identifierWOS:A1996WX73500003
dc.identifierhttp://dx.doi.org/10.1016/S0032-0633(96)00111-0
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/876075
dc.descriptionThe 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.
dc.languageeng
dc.publisherElsevier B.V.
dc.relationPlanetary and Space Science
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.title2060 Chiron back to a minimum of brightness
dc.typeOtro


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