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dc.contributor.authorMirabel, I. Felixpt_BR
dc.contributor.authorDottori, Horacio Albertopt_BR
dc.contributor.authorLutz, Dieterpt_BR
dc.date.accessioned2014-07-22T02:03:34Zpt_BR
dc.date.issued1992pt_BR
dc.identifier.issn0004-6361pt_BR
dc.identifier.urihttp://hdl.handle.net/10183/98351pt_BR
dc.description.abstractWe show that a dwarf irregular galaxy has formed out of the tidal remnants that were ejected to intergalactic space during an encounter of the disk galaxies NGC 4038/39 (the Antennae). The tidal dwarf consists of a chain of nebulae ionized by recently formed massive stars, which are embedded in an envelope of HI gas and low surface brightness optical emission. Since this object is at the tip of one of the tidal tails, star formation on a scale similar to star forming galaxies is taking place at ~ 100 kpc from the merging disks.en
dc.format.mimetypeapplication/pdf
dc.language.isoengpt_BR
dc.relation.ispartofAstronomy and Astrophysics. Berlin. Vol. 256, no. 1 (Mar. 1992), p. l19-l22pt_BR
dc.rightsOpen Accessen
dc.subjectGalaxies: formationen
dc.subjectAstrofisica extragalaticapt_BR
dc.subjectGaláxiaspt_BR
dc.subjectIrregularen
dc.subjectFormacao de estrelaspt_BR
dc.subjectNGC 4038/39en
dc.subjectFotometriapt_BR
dc.subjectHII regions: generalen
dc.subjectFotometria estelarpt_BR
dc.subjectAstronomia e astrofisicapt_BR
dc.titleGenesis of a dwarf galaxy from the debris of the antennaept_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb000056037pt_BR
dc.type.originEstrangeiropt_BR


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