activity
20102016
most citedChemistry in Infrared Dark Cloud Clumps: a Molecular Line Survey at 3 mm

213 citations · 617 across the 5 of their papers we have counts for

collaborators

5 papers

physics.space-ph2016★ 5 cited

Inverting OII 83.4 nm Dayglow Profiles Using Markov Chain Radiative Transfer

George Geddes, Ewan Douglas, Susanna C. Finn +2

Emission profiles of the resonantly scattered OII~83.4~nm triplet can in principle be used to estimate \(\mathrm{O}^+\) density profiles in the F2 region of the ionosphere. Given t…

astro-ph.GA2014★ 44 cited

Distributed Low-Mass Star Formation in the IRDC G34.43+00.24

Jonathan B. Foster, Héctor G. Arce, Marc Kassis +9

We have used deep near-infrared observations with adaptive optics to discover a distributed population of low-mass protostars within the filamentary Infrared Dark Cloud G34.43+00.2…

astro-ph.GA2012★ 213 cited

Chemistry in Infrared Dark Cloud Clumps: a Molecular Line Survey at 3 mm

Patricio Sanhueza, James M. Jackson, Jonathan B. Foster +3

We have observed 37 Infrared Dark Clouds (IRDCs), containing a total of 159 clumps, in high-density molecular tracers at 3 mm using the 22-meter ATNF Mopra Telescope located in Aus…

astro-ph.GA2011★ 153 cited

The Millimeter Astronomy Legacy Team 90 GHz (MALT90) Pilot Survey

Jonathan B. Foster, James M. Jackson, Elizabeth Barris +11

We describe a pilot survey conducted with the Mopra 22-m radio telescope in preparation for the Millimeter Astronomy Legacy Team Survey at 90 GHz (MALT90). We identified 182 candid…

astro-ph.GA2010★ 202 cited

The "Nessie" Nebula: Cluster Formation in a Filamentary Infrared Dark Cloud

James M. Jackson, Susanna C. Finn, Edward T. Chambers +2

The "Nessie" Nebula is a filamentary infrared dark cloud (IRDC) with a large aspect ratio of over 150:1 (1.5 degrees x 0.01 degrees, or 80 pc x 0.5 pc at a kinematic distance of 3.…