The Environments of Green Pea Galaxies. II. The Hα Dot Sample

We use spectroscopic redshifts obtained with the WIYN 3.5 m telescope to study the local galactic environment around 18 Green Pea (GP) galaxies. Our sample of GPs were discovered in the H α Dot Survey via their [O iii ] λ 5007 emission and span the redshift range 0.32 < z < 0.34. We present th...

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Main Authors: Brooke Kimsey-Miller, Samantha W. Brunker, John J. Salzer
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
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Online Access:https://doi.org/10.3847/1538-4357/ad8b4e
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author Brooke Kimsey-Miller
Samantha W. Brunker
John J. Salzer
author_facet Brooke Kimsey-Miller
Samantha W. Brunker
John J. Salzer
author_sort Brooke Kimsey-Miller
collection DOAJ
description We use spectroscopic redshifts obtained with the WIYN 3.5 m telescope to study the local galactic environment around 18 Green Pea (GP) galaxies. Our sample of GPs were discovered in the H α Dot Survey via their [O iii ] λ 5007 emission and span the redshift range 0.32 < z < 0.34. We present the environmental analyses near the location of the H α Dot GPs. We utilize three different density estimators, chosen based on the geometry of the redshift survey data within the H α Dot GP fields. We classify each H α Dot GP into an environment category, from extremely isolated to highly clustered. We find that our entire sample of H α Dot GPs reside in extremely isolated or low-density environments, with none located in the intermediate- to high-density regimes. We interpret this to indicate that major mergers and interactions do not drive the activity seen in these galaxies.
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spelling doaj-art-e5d39e0106dd46ebaf7c800b8e6062552024-12-04T08:01:41ZengIOP PublishingThe Astrophysical Journal1538-43572024-01-0197717910.3847/1538-4357/ad8b4eThe Environments of Green Pea Galaxies. II. The Hα Dot SampleBrooke Kimsey-Miller0https://orcid.org/0009-0005-6705-7073Samantha W. Brunker1https://orcid.org/0000-0001-6776-2550John J. Salzer2https://orcid.org/0000-0001-8483-603XDepartment of Astronomy, Indiana University , 727 East Third Street, Bloomington, IN 47405, USADepartment of Astronomy, Indiana University , 727 East Third Street, Bloomington, IN 47405, USADepartment of Astronomy, Indiana University , 727 East Third Street, Bloomington, IN 47405, USAWe use spectroscopic redshifts obtained with the WIYN 3.5 m telescope to study the local galactic environment around 18 Green Pea (GP) galaxies. Our sample of GPs were discovered in the H α Dot Survey via their [O iii ] λ 5007 emission and span the redshift range 0.32 < z < 0.34. We present the environmental analyses near the location of the H α Dot GPs. We utilize three different density estimators, chosen based on the geometry of the redshift survey data within the H α Dot GP fields. We classify each H α Dot GP into an environment category, from extremely isolated to highly clustered. We find that our entire sample of H α Dot GPs reside in extremely isolated or low-density environments, with none located in the intermediate- to high-density regimes. We interpret this to indicate that major mergers and interactions do not drive the activity seen in these galaxies.https://doi.org/10.3847/1538-4357/ad8b4eEmission line galaxiesLarge-scale structure of the universeRedshift surveysVoidsStarburst galaxiesGalaxy processes
spellingShingle Brooke Kimsey-Miller
Samantha W. Brunker
John J. Salzer
The Environments of Green Pea Galaxies. II. The Hα Dot Sample
The Astrophysical Journal
Emission line galaxies
Large-scale structure of the universe
Redshift surveys
Voids
Starburst galaxies
Galaxy processes
title The Environments of Green Pea Galaxies. II. The Hα Dot Sample
title_full The Environments of Green Pea Galaxies. II. The Hα Dot Sample
title_fullStr The Environments of Green Pea Galaxies. II. The Hα Dot Sample
title_full_unstemmed The Environments of Green Pea Galaxies. II. The Hα Dot Sample
title_short The Environments of Green Pea Galaxies. II. The Hα Dot Sample
title_sort environments of green pea galaxies ii the hα dot sample
topic Emission line galaxies
Large-scale structure of the universe
Redshift surveys
Voids
Starburst galaxies
Galaxy processes
url https://doi.org/10.3847/1538-4357/ad8b4e
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