125 citations · 1.3k across the 41 of their papers we have counts for
5 papers · 1 filter
The 21-SPONGE HI Absorption Line Survey II: The temperature of Galactic HI
Claire E. Murray, Snezana Stanimirovic, W. M. Goss +4
We present 21-cm Spectral Line Observations of Neutral Gas with the VLA (21-SPONGE), a Karl G. Jansky Very Large Array (VLA) large project (~600 hours) for measuring the physical p…
Optically thick HI does not dominate dark gas in the local ISM
Claire E. Murray, J. E. G. Peek, Min-Young Lee +1
The local interstellar medium (ISM) is suffused with "dark" gas, identified by excess infrared and gamma ray emission, yet undetected by standard ISM tracers such as neutral hydrog…
Dust-Gas Scaling Relations and OH Abundance in the Galactic ISM
Hiep Nguyen, J. R. Dawson, M. -A. Miville-Deschênes +10
Observations of interstellar dust are often used as a proxy for total gas column density . By comparing thermal dust data (Release 1.2) and new dust…
Calibrating the HISA temperature: Measuring the temperature of the Riegel-Crutcher cloud
H. Denes, N. M. McClure-Griffiths, J. M. Dickey +2
HI self absorption (HISA) clouds are clumps of cold neutral hydrogen (HI) visible in front of warm background gas, which makes them ideal places to study the properties of the cold…
Where is OH and Does It Trace the Dark Molecular Gas (DMG)?
Di Li, Ningyu Tang, Hiep Nguyen +15
Hydroxyl (OH) is expected to be abundant in diffuse interstellar molecular gas as it forms along with under similar conditions and within a similar extinction range. We have…