activity
20102024
most citedPlanck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds

422 citations · 3.5k across the 102 of their papers we have counts for

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Showing 2019Show all

8 papers · 1 filter

astro-ph.GA2019★ 64 cited

The HI/OH/Recombination line survey of the inner Milky Way (THOR): data release 2 and HI overview

Y. Wang, H. Beuther, M. R. Rugel +17

With the Very Large Array (VLA) in C-configuration, we observed a large portion of the first Galactic quadrant ( and $\lvert b \rvert \leq 1.25…

astro-ph.GA2019★ 38 cited

Strong excess Faraday rotation on the Inside of the Sagittarius spiral arm

R. Shanahan, S. J. Lemmer, J. M. Stil +12

We present first results for Faraday rotation of compact polarized sources (1 to 2 GHz continuum) in The HI/OH/Recombination line (THOR) survey of the inner Galaxy. In the Galactic…

astro-ph.SR2019★ 12 cited

Bow Magnetic Morphology Surrounding Filamentary Molecular Clouds? 3D Magnetic Field Structure of Orion-A

M. Tahani, R. Plume, J. C. Brown +2

Using a method based on Faraday rotation measurements, Tahani et al. 2018 find the line-of-sight component of magnetic fields in Orion-A and show that their direction changes from…

astro-ph.HE2019★ 36 cited

Gas shells and magnetic fields in the Orion-Eridanus superbubble

T. Joubaud, I. A. Grenier, J. Ballet +1

The Orion-Eridanus superbubble has been blown by supernovae and supersonic winds of the massive stars in the Orion OB associations. The formation history and current structure of t…

astro-ph.GA2019★ 93 cited

Using Herschel and Planck observations to delineate the role of magnetic fields in molecular cloud structure

Juan D. Soler

We present a study of the relative orientation between the magnetic field projected onto the plane of sky () on scales down to 0.4 pc, inferred from the polarized therma…

astro-ph.SR2019★ 39 cited

OH maser emission in the THOR survey of the northern Milky Way

H. Beuther, A. Walsh, Y. Wang +13

Context: OH masers trace diverse physical processes, from the expanding envelopes around evolved stars to star-forming regions or supernovae remnants. Aims: We identify the ground-…