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The Origins of [CII] Emission in Local Star-forming Galaxies
Kevin Croxall, J. D. T. Smith, Eric Pellegrini +17
The [CII] 158um fine-structure line is the brightest emission line observed in local star-forming galaxies. As a major coolant of the gas-phase interstellar medium, [CII] balances…
The Survey of Lines in M31 (SLIM): The Drivers of the [CII]/TIR Variation
Maria Julia Kapala, Brent Groves, Karin Sandstrom +7
The ratio of the [CII] 158m emission line over the total infrared emission (TIR) is often used as a proxy for the photoelectric (PE) heating efficiency () of the f…
Space Telescope and Optical Reverberation Mapping Project. VII. Understanding the UV anomaly in NGC 5548 with X-Ray Spectroscopy
S. Mathur, A. Gupta, K. Page +147
During the Space Telescope and Optical Reverberation Mapping Project (STORM) observations of NGC 5548, the continuum and emission-line variability became de-correlated during the s…
Space Telescope and Optical Reverberation Mapping Project. V. Optical Spectroscopic Campaign and Emission-Line Analysis for NGC 5548
L. Pei, M. M. Fausnaugh, A. J. Barth +153
We present the results of an optical spectroscopic monitoring program targeting NGC 5548 as part of a larger multi-wavelength reverberation mapping campaign. The campaign spanned s…
Thermal Pressure in the Cold Neutral Medium of Nearby Galaxies
R. Herrera-Camus, A. Bolatto, M. Wolfire +14
Dynamic and thermal processes regulate the structure of the multi-phase interstellar medium (ISM), and ultimately establish how galaxies evolve through star formation. Thus, to con…