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Title: [Ne III]/[O II] as an ionization parameter diagnostic in star-forming galaxies

Abstract

We present our parameterizations of the log([Ne III]λ3869/[O II]λ3727) (Ne3O2) and log([O III]λ5007/[O II]λ3727) (O3O2) ratios as diagnostics of ionization parameter in star-forming galaxies. Our calibrations are based on the Starburst99/Mappings III photoionization models, which extend up to the extremely high values of ionization parameter found in high-redshift galaxies. While similar calibrations have been presented previously for O3O2, this is the first such calibration of Ne3O2. We illustrate the tight correlation between these two ratios for star-forming galaxies and discuss the underlying physics that dictates their very similar evolution. Based on this work, we propose the Ne3O2 ratio as a new and useful diagnostic of ionization parameter for star-forming galaxies. Given the Ne3O2 ratio's relative insensitivity to reddening, this ratio is particularly valuable for use with galaxies that have uncertain amounts of extinction. The short wavelengths of the Ne3O2 ratio can also be applied out to very high redshifts, extending studies of galaxies' ionization parameters out to z ∼ 1.6 with optical spectroscopy and z ∼ 5.2 with ground-based near-infrared spectra.

Authors:
 [1];  [2]
  1. CASA, Department of Astrophysical and Planetary Sciences, University of Colorado 389-UCB, Boulder, CO 80309 (United States)
  2. School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287 (United States)
Publication Date:
OSTI Identifier:
22348274
Resource Type:
Journal Article
Resource Relation:
Journal Name: Astrophysical Journal; Journal Volume: 780; Journal Issue: 1; Other Information: Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; CALIBRATION; CORRELATIONS; EVOLUTION; GALAXIES; INFRARED SPECTRA; MAPPING; PHOTOIONIZATION; RED SHIFT; SPECTROSCOPY; STARS; WAVELENGTHS

Citation Formats

Levesque, Emily M., and Richardson, Mark L. A., E-mail: Emily.Levesque@colorado.edu. [Ne III]/[O II] as an ionization parameter diagnostic in star-forming galaxies. United States: N. p., 2014. Web. doi:10.1088/0004-637X/780/1/100.
Levesque, Emily M., & Richardson, Mark L. A., E-mail: Emily.Levesque@colorado.edu. [Ne III]/[O II] as an ionization parameter diagnostic in star-forming galaxies. United States. doi:10.1088/0004-637X/780/1/100.
Levesque, Emily M., and Richardson, Mark L. A., E-mail: Emily.Levesque@colorado.edu. Wed . "[Ne III]/[O II] as an ionization parameter diagnostic in star-forming galaxies". United States. doi:10.1088/0004-637X/780/1/100.
@article{osti_22348274,
title = {[Ne III]/[O II] as an ionization parameter diagnostic in star-forming galaxies},
author = {Levesque, Emily M. and Richardson, Mark L. A., E-mail: Emily.Levesque@colorado.edu},
abstractNote = {We present our parameterizations of the log([Ne III]λ3869/[O II]λ3727) (Ne3O2) and log([O III]λ5007/[O II]λ3727) (O3O2) ratios as diagnostics of ionization parameter in star-forming galaxies. Our calibrations are based on the Starburst99/Mappings III photoionization models, which extend up to the extremely high values of ionization parameter found in high-redshift galaxies. While similar calibrations have been presented previously for O3O2, this is the first such calibration of Ne3O2. We illustrate the tight correlation between these two ratios for star-forming galaxies and discuss the underlying physics that dictates their very similar evolution. Based on this work, we propose the Ne3O2 ratio as a new and useful diagnostic of ionization parameter for star-forming galaxies. Given the Ne3O2 ratio's relative insensitivity to reddening, this ratio is particularly valuable for use with galaxies that have uncertain amounts of extinction. The short wavelengths of the Ne3O2 ratio can also be applied out to very high redshifts, extending studies of galaxies' ionization parameters out to z ∼ 1.6 with optical spectroscopy and z ∼ 5.2 with ground-based near-infrared spectra.},
doi = {10.1088/0004-637X/780/1/100},
journal = {Astrophysical Journal},
number = 1,
volume = 780,
place = {United States},
year = {Wed Jan 01 00:00:00 EST 2014},
month = {Wed Jan 01 00:00:00 EST 2014}
}
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