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Direct Far-Infrared Metal Abundances (FIRA) I: M101
C. Lamarche, J. D. Smith, K. Kreckel +12
Accurately determining gas-phase metal-abundances within galaxies is critical as metals strongly affect the physics of the interstellar medium (ISM). To date, the vast majority of…
CHAOS VI: Direct Abundances in NGC 2403
Noah S. J. Rogers, Evan D. Skillman, Richard W. Pogge +4
We report the direct abundances for the galaxy NGC 2403 as observed by the CHemical Abundances Of Spirals (CHAOS) project. Using the Multi-Object Double Spectrograph on the Large B…
Characterizing the Multi-Phase Origin of [CII] Emission in M101 and NGC 6946 with Velocity Resolved Spectroscopy
Elizabeth Tarantino, Alberto D. Bolatto, Rodrigo Herrera-Camus +10
The [CII] fine-structure transition at 158 micron is frequently the brightest far-infrared line in galaxies. Due to its low ionization potential, C+ can trace the ionized, atomic,…
The Case for Thermalization as a Contributor to the [CII] Deficit
Jessica Sutter, Daniel A. Dale, Karin Sandstrom +15
The [CII] deficit, which describes the observed decrease in the ratio of [CII] 158 micron emission to continuum infrared emission in galaxies with high star formation surface densi…