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    The MOSDEF Survey: Neon as a Probe of ISM Physical Conditions at High Redshift

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    Jeong_2020_ApJL_902_L16.pdf
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    Final Published Version
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    Author
    Jeong, Moon-Seong
    Shapley, Alice E.
    Sanders, Ryan L.
    Runco, Jordan N.
    Topping, Michael W.
    Reddy, Naveen A.
    Kriek, Mariska cc
    Coil, Alison L.
    Mobasher, Bahram
    Siana, Brian cc
    Shivaei, Irene
    Freeman, William R.
    Azadi, Mojegan
    Price, Sedona H.
    Leung, Gene C. K.
    Fetherolf, Tara
    de Groot, Laura
    Zick, Tom
    Fornasini, Francesca M.
    Barro, Guillermo cc
    Show allShow less
    Affiliation
    Univ Arizona, Steward Observ
    Issue Date
    2020-10-08
    Keywords
    Galaxy evolution
    High-redshift galaxies
    Interstellar medium
    
    Metadata
    Show full item record
    Publisher
    IOP PUBLISHING LTD
    Citation
    Jeong, M. S., Shapley, A. E., Sanders, R. L., Runco, J. N., Topping, M. W., Reddy, N. A., ... & Barro, G. (2020). The MOSDEF Survey: Neon as a Probe of ISM Physical Conditions at High Redshift. The Astrophysical Journal Letters, 902(1), L16.
    Journal
    ASTROPHYSICAL JOURNAL LETTERS
    Rights
    © 2020. The American Astronomical Society. All rights reserved.
    Collection Information
    This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.
    Abstract
    We present results on the properties of neon emission inz similar to 2 star-forming galaxies drawn from the MOSFIRE Deep Evolution Field (MOSDEF) survey. Doubly ionized neon ([Neiii]lambda 3869) is detected at >= 3 sigma in 61 galaxies, representing similar to 25% of the MOSDEF sample with H alpha, H beta, and [Oiii]lambda 5007 detections at similar redshifts. We consider the neon emission-line properties of both individual galaxies with [Neiii]lambda 3869 detections and compositez similar to 2 spectra binned by stellar mass. With no requirement of [Neiii]lambda 3869 detection, the latter provide a more representative picture of neon emission-line properties in the MOSDEF sample. The [Neiii]lambda 3869/[Oii]lambda 3727 ratio (Ne3O2) is anticorrelated with stellar mass inz similar to 2 galaxies, as expected based on the mass-metallicity relation. It is also positively correlated with the [Oiii]lambda 5007/[Oii]lambda 3727 ratio (O32), butz similar to 2 line ratios are offset toward higher Ne3O2 at fixed O32, compared with both local star-forming galaxies and individual H iiregions. Despite the offset toward higher Ne3O2 at fixed O32 atz similar to 2, biases in inferred Ne3O2-based metallicity are small. Accordingly, Ne3O2 may serve as an important metallicity indicator deep into the reionization epoch. Analyzing additional rest-optical line ratios including [Neiii]lambda 3869/[Oiii]lambda 5007 (Ne3O3) and [Oiii]lambda 5007/H beta(O3H beta), we conclude that the nebular emission-line ratios ofz similar to 2 star-forming galaxies suggest a harder ionizing spectrum (lower stellar metallicity, i.e., Fe/H) at fixed gas-phase oxygen abundance, compared to systems atz similar to 0. These new results based on neon lend support to the physical picture painted by oxygen, nitrogen, hydrogen, and sulfur emission of an ionized interstellar medium in high-redshift star-forming galaxies irradiated by chemically young,alpha-enhanced massive stars.
    ISSN
    2041-8205
    EISSN
    2041-8213
    DOI
    10.3847/2041-8213/abba7a
    Version
    Final published version
    Sponsors
    Space Telescope Science Institute
    ae974a485f413a2113503eed53cd6c53
    10.3847/2041-8213/abba7a
    Scopus Count
    Collections
    UA Faculty Publications

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