Blueberry Galaxies: The Lowest Mass Young Starbursts

Searching for extreme emission line galaxies allows us to find low-mass metal-poor galaxies that are good analogs of high redshift Ly emitting galaxies. These low-mass extreme emission line galaxies are also potential Lyman-continuum leakers. Finding them at very low redshifts ( ) allows us to be se...

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Published inThe Astrophysical journal Vol. 847; no. 1; pp. 38 - 46
Main Authors Yang, Huan, Malhotra, Sangeeta, Rhoads, James E., Wang, Junxian
Format Journal Article
LanguageEnglish
Published Philadelphia The American Astronomical Society 20.09.2017
IOP Publishing
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Abstract Searching for extreme emission line galaxies allows us to find low-mass metal-poor galaxies that are good analogs of high redshift Ly emitting galaxies. These low-mass extreme emission line galaxies are also potential Lyman-continuum leakers. Finding them at very low redshifts ( ) allows us to be sensitive to even lower stellar masses and metallicities. We report on a sample of extreme emission line galaxies at (blueberry galaxies). We selected them from SDSS broadband images on the basis of their broadband colors and studied their properties with MMT spectroscopy. From the entire SDSS DR12 photometric catalog, we found 51 photometric candidates. We spectroscopically confirm 40 as blueberry galaxies. (An additional seven candidates are contaminants, and four remain without spectra.) These blueberries are dwarf starburst galaxies with very small sizes (<1 kpc) and very high ionization ([O iii]/[O ii] ∼ 10-60). They also have some of the lowest stellar masses ( ) and lowest metallicities ( ) of starburst galaxies. Thus, they are small counterparts to green pea galaxies and high redshift Ly emitting galaxies.
AbstractList Searching for extreme emission line galaxies allows us to find low-mass metal-poor galaxies that are good analogs of high redshift Lyα emitting galaxies. These low-mass extreme emission line galaxies are also potential Lyman-continuum leakers. Finding them at very low redshifts (z≲0.05) allows us to be sensitive to even lower stellar masses and metallicities. We report on a sample of extreme emission line galaxies at z≲0.05 (blueberry galaxies). We selected them from SDSS broadband images on the basis of their broadband colors and studied their properties with MMT spectroscopy. From the entire SDSS DR12 photometric catalog, we found 51 photometric candidates. We spectroscopically confirm 40 as blueberry galaxies. (An additional seven candidates are contaminants, and four remain without spectra.) These blueberries are dwarf starburst galaxies with very small sizes (<1 kpc) and very high ionization ([O iii]/[O ii] ∼ 10–60). They also have some of the lowest stellar masses (log(M/M{sub ⊙})∼6.5--7.5) and lowest metallicities (7.1<12+log(O/H)<7.8) of starburst galaxies. Thus, they are small counterparts to green pea galaxies and high redshift Lyα emitting galaxies.
Abstract Searching for extreme emission line galaxies allows us to find low-mass metal-poor galaxies that are good analogs of high redshift Ly α emitting galaxies. These low-mass extreme emission line galaxies are also potential Lyman-continuum leakers. Finding them at very low redshifts ( ) allows us to be sensitive to even lower stellar masses and metallicities. We report on a sample of extreme emission line galaxies at (blueberry galaxies). We selected them from SDSS broadband images on the basis of their broadband colors and studied their properties with MMT spectroscopy. From the entire SDSS DR12 photometric catalog, we found 51 photometric candidates. We spectroscopically confirm 40 as blueberry galaxies. (An additional seven candidates are contaminants, and four remain without spectra.) These blueberries are dwarf starburst galaxies with very small sizes (<1 kpc) and very high ionization ([O iii ]/[O ii ] ∼ 10–60). They also have some of the lowest stellar masses ( ) and lowest metallicities ( ) of starburst galaxies. Thus, they are small counterparts to green pea galaxies and high redshift Ly α emitting galaxies.
Searching for extreme emission line galaxies allows us to find low-mass metal-poor galaxies that are good analogs of high redshift Ly emitting galaxies. These low-mass extreme emission line galaxies are also potential Lyman-continuum leakers. Finding them at very low redshifts ( ) allows us to be sensitive to even lower stellar masses and metallicities. We report on a sample of extreme emission line galaxies at (blueberry galaxies). We selected them from SDSS broadband images on the basis of their broadband colors and studied their properties with MMT spectroscopy. From the entire SDSS DR12 photometric catalog, we found 51 photometric candidates. We spectroscopically confirm 40 as blueberry galaxies. (An additional seven candidates are contaminants, and four remain without spectra.) These blueberries are dwarf starburst galaxies with very small sizes (<1 kpc) and very high ionization ([O iii]/[O ii] ∼ 10-60). They also have some of the lowest stellar masses ( ) and lowest metallicities ( ) of starburst galaxies. Thus, they are small counterparts to green pea galaxies and high redshift Ly emitting galaxies.
Searching for extreme emission line galaxies allows us to find low-mass metal-poor galaxies that are good analogs of high redshift Lyα emitting galaxies. These low-mass extreme emission line galaxies are also potential Lyman-continuum leakers. Finding them at very low redshifts (\(z\lesssim 0.05\)) allows us to be sensitive to even lower stellar masses and metallicities. We report on a sample of extreme emission line galaxies at \(z\lesssim 0.05\) (blueberry galaxies). We selected them from SDSS broadband images on the basis of their broadband colors and studied their properties with MMT spectroscopy. From the entire SDSS DR12 photometric catalog, we found 51 photometric candidates. We spectroscopically confirm 40 as blueberry galaxies. (An additional seven candidates are contaminants, and four remain without spectra.) These blueberries are dwarf starburst galaxies with very small sizes (<1 kpc) and very high ionization ([O iii]/[O ii] ∼ 10–60). They also have some of the lowest stellar masses (\(\mathrm{log}(M/{M}_{\odot })\sim 6.5\mbox{--}7.5\)) and lowest metallicities (\(7.1\lt 12+\mathrm{log}({\rm{O}}/{\rm{H}})\lt 7.8\)) of starburst galaxies. Thus, they are small counterparts to green pea galaxies and high redshift Lyα emitting galaxies.
Author Wang, Junxian
Rhoads, James E.
Yang, Huan
Malhotra, Sangeeta
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  givenname: Junxian
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  surname: Wang
  fullname: Wang, Junxian
  organization: University of Science and Technology of China CAS Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, China
BackLink https://www.osti.gov/biblio/22875776$$D View this record in Osti.gov
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Copyright 2017. The American Astronomical Society. All rights reserved.
Copyright IOP Publishing Sep 20, 2017
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Snippet Searching for extreme emission line galaxies allows us to find low-mass metal-poor galaxies that are good analogs of high redshift Ly emitting galaxies. These...
Abstract Searching for extreme emission line galaxies allows us to find low-mass metal-poor galaxies that are good analogs of high redshift Ly α emitting...
Searching for extreme emission line galaxies allows us to find low-mass metal-poor galaxies that are good analogs of high redshift Lyα emitting galaxies. These...
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SubjectTerms Analogs
Astrophysics
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
Blueberries
Broadband
Contaminants
Dwarf galaxies
EMISSION
Emission lines
GALAXIES
galaxies: dwarf
galaxies: high-redshift
galaxies: ISM
galaxies: star formation
galaxies: starburst
IONIZATION
LYMAN LINES
MASS
METALLICITY
Photometry
RED SHIFT
regions
SPECTRA
Spectroscopy
Spectrum analysis
STAR EVOLUTION
Starburst galaxies
STARS
Stars & galaxies
Title Blueberry Galaxies: The Lowest Mass Young Starbursts
URI https://iopscience.iop.org/article/10.3847/1538-4357/aa8809
https://www.proquest.com/docview/2365780311
https://www.osti.gov/biblio/22875776
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