222 citations · 528 across the 9 of their papers we have counts for
9 papers
A Survey of Magnetic Field Strengths in the Envelopes of Molecular Clouds via the 18 cm OH Zeeman Effect
K. L. Thompson, T. H. Troland, C. Heiles
We present the results of an extensive Arecibo observational survey of magnetic field strengths in the inter-core regions of molecular clouds to determine their role in the evoluti…
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…
Herschel dust emission as a probe of starless cores mass: MCLD 123.5+24.9 of the Polaris Flare
Gururaj A. Wagle, Thomas H. Troland, Gary J. Ferland +1
We present newly processed archival Herschel images of molecular cloud MCLD 123.5+24.9 in the Polaris Flare. This cloud contains five starless cores. Using the spectral synthesis c…
Response to the Mouschovias-Tassis Comments on "Testing Magnetic Star Formation Theory"
Richard M. Crutcher, Nicholas Hakobian, Thomas H. Troland
In this note we respond to Mouschovias and Kassis criticisms that our paper "Testing Magnetic Star Formation Theory" is flawed. We stand fully behind our paper.
Testing Magnetic Star Formation Theory
Richard M. Crutcher, Nicholas Hakobian, Thomas H. Troland
We report here observations of the Zeeman effect in the 18-cm lines of OH in the envelope regions surrounding four molecular cloud cores toward which detections of B(LOS) have been…