activity
20122019
most citedThe JCMT BISTRO Survey: The magnetic field strength in the Orion A filament

144 citations · 538 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.GA201960 cited

The JCMT BISTRO Survey: The Magnetic Field of the Barnard 1 Star-Forming Region

Simon Coudé, Pierre Bastien, Martin Houde +118

We present the POL-2 850 m linear polarization map of the Barnard 1 clump in the Perseus molecular cloud complex from the B-fields In STar-forming Region Observations (BISTRO) s…

astro-ph.GA201822 cited

Similar complex kinematics within two massive, filamentary infrared dark clouds

A. T. Barnes, J. D. Henshaw, P. Caselli +5

Infrared dark clouds (IRDCs) are thought to be potential hosts of the elusive early phases of high-mass star formation. Here we conduct an in-depth kinematic analysis of one such I…

astro-ph.SR201768 cited

How do stars gain their mass? A JCMT/SCUBA-2 Transient Survey of Protostars in Nearby Star Forming Regions

Gregory J. Herczeg, Doug Johnstone, Steve Mairs +55

Most protostars have luminosities that are fainter than expected from steady accretion over the protostellar lifetime. The solution to this problem may lie in episodic mass accreti…

astro-ph.EP2017140 cited

Seeds of Life in Space (SOLIS) III. Formamide in protostellar shocks: evidence for gas-phase formation

C. Codella, C. Ceccarelli, P. Caselli +47

Context: Modern versions of the Miller-Urey experiment claim that formamide (NHCHO) could be the starting point for the formation of metabolic and genetic macromolecules. Intri…

astro-ph.GA2017144 cited

The JCMT BISTRO Survey: The magnetic field strength in the Orion A filament

Kate Pattle, Derek Ward-Thompson, David Berry +27

We determine the magnetic field strength in the OMC 1 region of the Orion A filament via a new implementation of the Chandrasekhar-Fermi method using observations performed as part…

astro-ph.GA201513 cited

Mid-J CO Shock Tracing Observations of Infrared Dark Clouds I

A. Pon, P. Caselli, D. Johnstone +5

Infrared dark clouds (IRDCs) are dense, molecular structures in the interstellar medium that can harbour sites of high-mass star formation. IRDCs contain supersonic turbulence, whi…