62 citations · 332 across the 23 of their papers we have counts for
23 papers
Constraints on the properties of warm ionized gas from low-frequency hydrogen radio recombination lines
Pedro Salas, Kimberly L. Emig, Matteo Luisi +2
The ionized gas in the Milky Way is a major component of the interstellar medium. Observations of extinction free tracers, such as hydrogen radio recombination lines (HRRLs), have…
Expansion Signatures in 35 HII Regions traced by SOFIA [CII] Emission
Timothy Faerber, Loren D. Anderson, Matteo Luisi +6
We analyze the expansion signatures of 35 HII regions mapped in [CII] 158 micron emission by the Stratospheric Observatory for Infrared Astronomy (SOFIA). The [CII] emission primar…
Cool dark gas in Cygnus X: The first large-scale mapping of low-frequency carbon recombination lines
Kimberly L. Emig, Pedro Salas, Loren D. Anderson +14
Understanding the transition from atomic gas to molecular gas is critical to explain the formation and evolution of molecular clouds. However, the gas phases involved, cold HI and…
Nitrogen Abundance Distribution in the inner Milky Way
Jorge L. Pineda, Shinji Horiuchi, L. D. Anderson +9
We combine a new Galactic plane survey of Hydrogen Radio Recombination Lines (RRLs) with far-infrared (FIR) surveys of ionized Nitrogen, N+, to determine Nitrogen abundance across…
The Most Sensitive Radio Recombination Line Measurements Ever Made of the Galactic Warm Ionized Medium
T. M. Bania, Dana S. Balser, Trey V. Wenger +3
Diffuse ionized gas pervades the disk of the Milky Way. We detect extremely faint emission from this Galactic Warm Ionized Medium (WIM) using the Green Bank Telescope to make radio…
Low-frequency absorption and radio recombination line features of the Galactic Center Lobe
Natasha Hurley-Walker, L. D. Anderson, M. Luisi +6
The Galactic center lobe (GCL) is a object located north of the Galactic center. In the mid-infrared (MIR), the GCL appears as two 8.0-micron filaments that roughly…