We examine how the cosmic environment affects the chemical evolution of galaxies in the universe by comparing the N/O ratio of dwarf galaxies in voids with that of dwarf galaxies in denser regions. Ratios of the forbidden [O III] and [S II] transitions provide estimates of a region's electron temperature and number density. We estimate the abundances of oxygen and nitrogen using these temperature and density estimates and the emission-line fluxes [O II] lambda 3727, [O III] lambda lambda 4959, 5007, and [N II] lambda lambda 6548, 6584 with the direct T-e method. Using spectroscopic observations from the Sloan Digital Sky Survey Data Release 7, we are able to estimate the N/O ratio in 42 void dwarf galaxies and 89 dwarf galaxies in denser regions. The N/O ratio for void dwarfs (M-r > -17) is slightly lower (similar to 12%) than for dwarf galaxies in denser regions. We also estimate the nitrogen and oxygen abundances of 2050 void galaxies and 3883 galaxies in denser regions with M-r > -20. These somewhat brighter galaxies (but still fainter than L*) also display similar minor shifts in the N/O ratio. The shifts in the average and median element abundance values in all absolute magnitude bins studied are in the same direction, suggesting that the large-scale environment may influence the chemical evolution of galaxies. We discuss possible causes of such a large-scale environmental dependence of the chemical evolution of galaxies, including retarded star formation and a higher ratio of dark matter halo mass to stellar mass in void galaxies.
Large-scale Environmental Dependence of the Abundance Ratio of Nitrogen to Oxygen in Blue, Star-forming Galaxies Fainter than L-
Creators
Kelly A. Douglass - Drexel Univ, Dept Phys, 3141 Chestnut St, Philadelphia, PA 19104 USA
Michael S. Vogeley - Drexel University
Publication Details
The Astrophysical journal, v 837(1)
Publisher
Iop Publishing Ltd
Number of pages
14
Grant note
Max Planck Society; Foundation CELLEX
University of Cambridge
University of Chicago
Max-Planck-Institute for Astrophysics (MPA)
U.S. Department of Energy; United States Department of Energy (DOE)
National Aeronautics and Space Administration; National Aeronautics & Space Administration (NASA)
University of Basil
Korean Scientist Group
Institute for Advanced Study
Chinese Academy of Sciences (LAMOST); Chinese Academy of Sciences
United States Naval Observatory
1410525 / Direct For Mathematical & Physical Scien; National Science Foundation (NSF); NSF - Directorate for Mathematical & Physical Sciences (MPS)
Japanese Monbukagakusho; Ministry of Education, Culture, Sports, Science and Technology, Japan (MEXT)
Ohio State University
Fermilab
1430152 / Division Of Physics; National Science Foundation (NSF); NSF - Directorate for Mathematical & Physical Sciences (MPS)
University of Pittsburgh
Los Alamos National Laboratory; United States Department of Energy (DOE)
Joint Institute for Nuclear Astrophysics
Alfred P. Sloan Foundation
University of Washington
Princeton University
Max-Planck-Institute for Astronomy (MPIA)
New Mexico State University
Japan Participation Group; Sloan Digital Sky Survey (SDSS)
University of Portsmouth
Higher Education Funding Council for England; UK Research & Innovation (UKRI); Higher Education Funding Council for England (HEFCE)
Astrophysical Institute Potsdam
Kavli Institute for Particle Astrophysics and Cosmology
American Museum of Natural History
Case Western Reserve University
AST-1410525 / NSF; National Science Foundation (NSF)
National Science Foundation; National Science Foundation (NSF)
Johns Hopkins University
Drexel University
Resource Type
Journal article
Language
English
Academic Unit
Physics
Web of Science ID
WOS:000395918600007
Scopus ID
2-s2.0-85015206052
Other Identifier
991019167917004721
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