Kevin V. Croxall, Ph.D.
Affiliations: | 2010 | Astronomy | Indiana University, Bloomington, Bloomington, IN, United States |
Area:
Astrophysics PhysicsGoogle:
"Kevin Croxall"Parents
Sign in to add mentorLiese Ellen van Zee | grad student | 2010 | Indiana University Bloomington | |
(The chemical evolution of galaxies in the local volume.) | ||||
Richard William Pogge | post-doc | 2012-2016 | Ohio State |
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Publications
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Skillman ED, Berg DA, Pogge RW, et al. (2020) CHAOS V: Recombination Line Carbon Abundances in M 101 The Astrophysical Journal. 894: 138 |
Berg DA, Pogge RW, Skillman ED, et al. (2020) CHAOS IV: Gas-phase Abundance Trends from the First Four CHAOS Galaxies The Astrophysical Journal. 893: 96 |
Sutter J, Dale DA, Croxall KV, et al. (2019) Using [C ii] 158 μm Emission from Isolated ISM Phases as a Star Formation Rate Indicator The Astrophysical Journal. 886: 60 |
Howk JC, Rueff KM, Lehner N, et al. (2018) Extraplanar H ii Regions in Spiral Galaxies. I. Low-metallicity Gas Accreting through the Disk-halo Interface of NGC 4013 The Astrophysical Journal. 856: 166 |
Howk JC, Rueff KM, Lehner N, et al. (2018) Extraplanar H ii Regions in Spiral Galaxies. II. In Situ Star Formation in the Interstellar Thick Disk of NGC 4013 The Astrophysical Journal. 856: 167 |
Jameson KE, Bolatto AD, Wolfire M, et al. (2018) First Results from theHerscheland ALMA Spectroscopic Surveys of the SMC: The Relationship between [C ii]-bright Gas and CO-bright Gas at Low Metallicity The Astrophysical Journal. 853: 111 |
Kapala MJ, Groves B, Sandstrom K, et al. (2017) The Survey of Lines in M31 (SLIM): The Drivers of the [C ii]/TIR Variation The Astrophysical Journal. 842: 128 |
Smith JDT, Croxall K, Draine B, et al. (2016) THE SPATIALLY RESOLVED $[{\rm{C}}\,{\rm{ii}}]$ COOLING LINE DEFICIT IN GALAXIES The Astrophysical Journal. 834: 5 |
Croxall KV, Pogge RW, Berg DA, et al. (2016) Chaos. Iii. Gas-Phase Abundances In Ngc 5457 The Astrophysical Journal. 830: 4 |
Hirschauer AS, Salzer JJ, Skillman ED, et al. (2016) ALFALFA DISCOVERY of the MOST METAL-POOR GAS-RICH GALAXY KNOWN: AGC 198691 Astrophysical Journal. 822 |