Z-FIRE: ISM Properties of the z = 2.095 Cosmos Cluster

Article


Kewley, Lisa J., Yuan, Tiantian, Nanayakkara, Themiya, Kacprzak, Glenn G., Tran, Kim-Vy H., Glazebrook, Karl, Spitler, Lee, Cowley, Michael, Dopita, Michael, Straatman, Caroline, Labbé, Ivo and Tomczak, Adam. 2016. "Z-FIRE: ISM Properties of the z = 2.095 Cosmos Cluster." The Astrophysical Journal: an international review of astronomy and astronomical physics. 819 (2), pp. 1-10. https://doi.org/10.3847/0004-637X/819/2/100
Article Title

Z-FIRE: ISM Properties of the z = 2.095 Cosmos Cluster

ERA Journal ID1057
Article CategoryArticle
AuthorsKewley, Lisa J., Yuan, Tiantian, Nanayakkara, Themiya, Kacprzak, Glenn G., Tran, Kim-Vy H., Glazebrook, Karl, Spitler, Lee, Cowley, Michael, Dopita, Michael, Straatman, Caroline, Labbé, Ivo and Tomczak, Adam
Journal TitleThe Astrophysical Journal: an international review of astronomy and astronomical physics
Journal Citation819 (2), pp. 1-10
Article Number100
Number of Pages10
Year2016
PublisherIOP Publishing
Place of PublicationUnited States
ISSN0004-637X
1538-4357
Digital Object Identifier (DOI)https://doi.org/10.3847/0004-637X/819/2/100
Web Address (URL)https://iopscience.iop.org/article/10.3847/0004-637X/819/2/100
Abstract

We investigate the ISM properties of 13 star-forming galaxies within the z ∼ 2 COSMOS cluster. We show that the cluster members have [N II]/Hα and [O III]/Hβ emission-line ratios similar to z ∼ 2 field galaxies, yet systematically different emission-line ratios (by ∼0.17 dex) from the majority of local star-forming galaxies. We find no statistically significant difference in the [N II]/Hα and [O III]/Hβ line ratios or ISM pressures among the z ∼ 2 cluster galaxies and field galaxies at the same redshift. We show that our cluster galaxies have significantly larger ionization parameters (by up to an order of magnitude) than local star-forming galaxies. We hypothesize that these high ionization parameters may be associated with large specific star formation rates (SFRs; i.e., a large SFR per unit stellar mass). If this hypothesis is correct, then this relationship would have important implications for the geometry and/or the mass of stars contained within individual star clusters as a function of redshift.

Keywordsgalaxies: abundances; galaxies: fundamental parameters; galaxies: starburst
Contains Sensitive ContentDoes not contain sensitive content
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Byline AffiliationsAustralian National University
Swinburne University of Technology
Texas A&M University, United States
Macquarie University
Australian Astronomical Observatory, Australia
King Abdulaziz University, Saudi Arabia
Leiden University, Netherlands
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