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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/35392
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dc.contributor.authorFagundes, H.-
dc.date.accessioned2014-05-20T15:24:52Z-
dc.date.accessioned2016-10-25T17:59:11Z-
dc.date.available2014-05-20T15:24:52Z-
dc.date.available2016-10-25T17:59:11Z-
dc.date.issued1990-11-01-
dc.identifierhttp://adsabs.harvard.edu/full/1990RMxAA..21...79F-
dc.identifier.citationRevista Mexicana de Astronomia Y Astrofisica. Mexico City: Univ Nacional Autonoma Mexico, Inst de Astronomia, v. 21, n. SI, p. 79-83, 1990.-
dc.identifier.issn0185-1101-
dc.identifier.urihttp://hdl.handle.net/11449/35392-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/35392-
dc.description.abstractThe alignment of a pair of QSO triplets discovered by Arp and Hazard are tentatively explained by a combination of (I) the idea of quasar ejection by galaxies; (II) a construction by Narlikar suggesting a common origin for the six images; and (III) a nontrivial topology of cosmic space.en
dc.format.extent79-83-
dc.language.isoeng-
dc.publisherUniv Nacional Autonoma Mexico, Inst de Astronomia-
dc.sourceWeb of Science-
dc.subjectGRAVITATIONpt
dc.subjectQUASARSpt
dc.titleA SUGGESTION ON THE PAIR OF QSO TRIPLETS 1130+106 (B,A,C), (X,Y,Z)en
dc.typeoutro-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationUNIV ESTADUAL PAULISTA,INST FIS TEOR,RUA PAMPLONA 145,BR-01405 SAO PAULO,BRAZIL-
dc.description.affiliationUnespUNIV ESTADUAL PAULISTA,INST FIS TEOR,RUA PAMPLONA 145,BR-01405 SAO PAULO,BRAZIL-
dc.identifier.wosWOS:A1990EM94300016-
dc.rights.accessRightsAcesso aberto-
dc.identifier.fileWOSA1990EM94300016.pdf-
dc.relation.ispartofRevista Mexicana de Astronomia Y Astrofisica-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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