285 citations · 3.8k across the 84 of their papers we have counts for
6 papers · 1 filter
Atomic and Ionized Microstructures in the Diffuse Interstellar Medium
Snezana Stanimirovic, Ellen G. Zweibel
It has been known for half a century that the interstellar medium (ISM) of our Galaxy is structured on scales as small as a few hundred km, more than 10 orders of magnitude smaller…
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…
Kinematics of the Atomic ISM in M33 on 80 pc scales
Eric W. Koch, Erik W. Rosolowsky, Felix J. Lockman +7
We present new L-band ($1\mbox{--}2$ GHz) observations of the nearby spiral galaxy M33 with 80 pc resolution obtained with the Karl G. Jansky Very Large Array. The HI observations,…
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…
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…