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The Spatially Resolved [CII] Cooling Line Deficit in Galaxies
J. D. T. Smith, Kevin Croxall, Bruce Draine +17
We present [CII] 158um measurements from over 15,000 resolved regions within 54 nearby galaxies of the KINGFISH program to investigate the so-called [CII] "line cooling deficit" lo…
A Simple and Accurate Network for Hydrogen and Carbon Chemistry in the ISM
Munan Gong, Eve C. Ostriker, Mark G. Wolfire
Chemistry plays an important role in the interstellar medium (ISM), regulating heating and cooling of the gas, and determining abundances of molecular species that trace gas proper…
The chemistry of interstellar argonium and other probes of the molecular fraction in diffuse clouds
David A. Neufeld, Mark G. Wolfire
We present a general parameter study, in which the abundance of interstellar argonium (ArH) is predicted using a model for the physics and chemistry of diffuse interstellar gas…
The Ionized Gas in Nearby Galaxies as Traced by the [NII] 122 and 205 μm Transitions
R. Herrera-Camus, A. Bolatto, J. D. Smith +20
The [NII] 122 and 205 μm transitions are powerful tracers of the ionized gas in the interstellar medium. By combining data from 21 galaxies selected from the Herschel KINGFISH and…