Galaxy properties in different environments. I. The sample
Autor(a) principal: | |
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Data de Publicação: | 1994 |
Outros Autores: | , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UFRGS |
Texto Completo: | http://hdl.handle.net/10183/109047 |
Resumo: | This 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. |
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Maia, Marcio Antonio GeimbaPastoriza, Miriani GriseldaBica, Eduardo Luiz DamianiDottori, Horacio Alberto2015-01-20T02:15:11Z19940067-0049http://hdl.handle.net/10183/109047000256594This 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.application/pdfengThe Astrophysical journal. Supplement series. Chicago. Vol. 93, no. 2 (Aug. 1994), p. 425-440Astrofisica extragalaticaMateria interestelarFormacao de estrelasGaláxias ativasGalaxias seyfertGalaxies: clusteringGalaxies: structureGalaxy properties in different environments. I. The sampleEstrangeiroinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/openAccessreponame:Repositório Institucional da UFRGSinstname:Universidade Federal do Rio Grande do Sul (UFRGS)instacron:UFRGSORIGINAL000256594.pdf000256594.pdfTexto completo (inglês)application/pdf348296http://www.lume.ufrgs.br/bitstream/10183/109047/1/000256594.pdf8890bffcf59b6cd9cc3a7d505c50b99aMD51TEXT000256594.pdf.txt000256594.pdf.txtExtracted Texttext/plain352http://www.lume.ufrgs.br/bitstream/10183/109047/2/000256594.pdf.txtdc6dd52868d3b6fc2be621c43b46837bMD52THUMBNAIL000256594.pdf.jpg000256594.pdf.jpgGenerated Thumbnailimage/jpeg2057http://www.lume.ufrgs.br/bitstream/10183/109047/3/000256594.pdf.jpg97ed22fcb9dbc85ad9bd6605a12b0487MD5310183/1090472024-04-11 06:24:52.009502oai:www.lume.ufrgs.br:10183/109047Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2024-04-11T09:24:52Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false |
dc.title.pt_BR.fl_str_mv |
Galaxy properties in different environments. I. The sample |
title |
Galaxy properties in different environments. I. The sample |
spellingShingle |
Galaxy properties in different environments. I. The sample Maia, Marcio Antonio Geimba Astrofisica extragalatica Materia interestelar Formacao de estrelas Galáxias ativas Galaxias seyfert Galaxies: clustering Galaxies: structure |
title_short |
Galaxy properties in different environments. I. The sample |
title_full |
Galaxy properties in different environments. I. The sample |
title_fullStr |
Galaxy properties in different environments. I. The sample |
title_full_unstemmed |
Galaxy properties in different environments. I. The sample |
title_sort |
Galaxy properties in different environments. I. The sample |
author |
Maia, Marcio Antonio Geimba |
author_facet |
Maia, Marcio Antonio Geimba Pastoriza, Miriani Griselda Bica, Eduardo Luiz Damiani Dottori, Horacio Alberto |
author_role |
author |
author2 |
Pastoriza, Miriani Griselda Bica, Eduardo Luiz Damiani Dottori, Horacio Alberto |
author2_role |
author author author |
dc.contributor.author.fl_str_mv |
Maia, Marcio Antonio Geimba Pastoriza, Miriani Griselda Bica, Eduardo Luiz Damiani Dottori, Horacio Alberto |
dc.subject.por.fl_str_mv |
Astrofisica extragalatica Materia interestelar Formacao de estrelas Galáxias ativas Galaxias seyfert |
topic |
Astrofisica extragalatica Materia interestelar Formacao de estrelas Galáxias ativas Galaxias seyfert Galaxies: clustering Galaxies: structure |
dc.subject.eng.fl_str_mv |
Galaxies: clustering Galaxies: structure |
description |
This 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. |
publishDate |
1994 |
dc.date.issued.fl_str_mv |
1994 |
dc.date.accessioned.fl_str_mv |
2015-01-20T02:15:11Z |
dc.type.driver.fl_str_mv |
Estrangeiro info:eu-repo/semantics/article |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://hdl.handle.net/10183/109047 |
dc.identifier.issn.pt_BR.fl_str_mv |
0067-0049 |
dc.identifier.nrb.pt_BR.fl_str_mv |
000256594 |
identifier_str_mv |
0067-0049 000256594 |
url |
http://hdl.handle.net/10183/109047 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.ispartof.pt_BR.fl_str_mv |
The Astrophysical journal. Supplement series. Chicago. Vol. 93, no. 2 (Aug. 1994), p. 425-440 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
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application/pdf |
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