GALAXY PROPERTIES IN DIFFERENT ENVIRONMENTS .1. THE SAMPLE
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MAIA, MAG
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UNIV FED RIO GRANDE DO SUL,INST FIS,DEPT ASTRON,BR-91501970 PORTO ALEGRE,RS,BRAZILUNIV FED RIO GRANDE DO SUL,INST FIS,DEPT ASTRON,BR-91501970 PORTO ALEGRE,RS,BRAZIL
MAIA, MAG
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PASTORIZA, MG
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UNIV FED RIO GRANDE DO SUL,INST FIS,DEPT ASTRON,BR-91501970 PORTO ALEGRE,RS,BRAZILUNIV FED RIO GRANDE DO SUL,INST FIS,DEPT ASTRON,BR-91501970 PORTO ALEGRE,RS,BRAZIL
PASTORIZA, MG
[1
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BICA, E
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UNIV FED RIO GRANDE DO SUL,INST FIS,DEPT ASTRON,BR-91501970 PORTO ALEGRE,RS,BRAZILUNIV FED RIO GRANDE DO SUL,INST FIS,DEPT ASTRON,BR-91501970 PORTO ALEGRE,RS,BRAZIL
BICA, E
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DOTTORI, H
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UNIV FED RIO GRANDE DO SUL,INST FIS,DEPT ASTRON,BR-91501970 PORTO ALEGRE,RS,BRAZILUNIV FED RIO GRANDE DO SUL,INST FIS,DEPT ASTRON,BR-91501970 PORTO ALEGRE,RS,BRAZIL
DOTTORI, H
[1
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机构:
[1] UNIV FED RIO GRANDE DO SUL,INST FIS,DEPT ASTRON,BR-91501970 PORTO ALEGRE,RS,BRAZIL
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.