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dc.contributor.authorMaia, Marcio Antonio Geimbapt_BR
dc.contributor.authorPastoriza, Miriani Griseldapt_BR
dc.contributor.authorBica, Eduardo Luiz Damianipt_BR
dc.contributor.authorDottori, Horacio Albertopt_BR
dc.date.accessioned2015-01-20T02:15:11Zpt_BR
dc.date.issued1994pt_BR
dc.identifier.issn0067-0049pt_BR
dc.identifier.urihttp://hdl.handle.net/10183/109047pt_BR
dc.description.abstractThis paper presents two galaxy samples, respectively in a high and in a low local density environments that were generated from the SSRS catalog using objective criteria. A preliminary comparison of physical properties in these two samples reveals that galaxies in high-density environments tend to be under a higher starbursting activity, have a deficiency of the neutral hydrogen content, present a higher fractional Seyfert population and a higher fraction of barred spirals as well. The present samples are intended to be used in future spectroscopic observations for more detailed investigation.en
dc.format.mimetypeapplication/pdf
dc.language.isoengpt_BR
dc.relation.ispartofThe Astrophysical journal. Supplement series. Chicago. Vol. 93, no. 2 (Aug. 1994), p. 425-440pt_BR
dc.rightsOpen Accessen
dc.subjectAstrofisica extragalaticapt_BR
dc.subjectGalaxies: clusteringen
dc.subjectGalaxies: structureen
dc.subjectMateria interestelarpt_BR
dc.subjectFormacao de estrelaspt_BR
dc.subjectGaláxias ativaspt_BR
dc.subjectGalaxias seyfertpt_BR
dc.titleGalaxy properties in different environments. I. The samplept_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb000256594pt_BR
dc.type.originEstrangeiropt_BR


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