10 citations · 14 across the 5 of their papers we have counts for
5 papers
Dense Molecular Clumps with Large Blue Asymmetries: Evidence for Collapse
James M. Jackson, J. Scott Whitaker, Edward Chambers +10
An analysis of the Millimetre Astronomy Legacy Team 90 GHz (MALT90) survey has produced a sample of 27 candidate dense molecular clumps with large collapse motions, as revealed by…
Absorption and Self-Absorption of [C II] and [O I] Far Infrared Lines Towards a Bright Bubble in the Nessie Infrared Dark Cloud
J. M. Jackson, J. S. Whitaker, E. T. Chambers +15
Using the upGREAT instrument on SOFIA, we have imaged [C II] 157.74 and [O I] 63.18 micron line emission from a bright photodissociation region (PDR) associated with an ionized ``b…
The MACH HI absorption survey I: Physical conditions of cold atomic gas outside of the Galactic plane
Claire E. Murray, Snežana Stanimirović, Carl Heiles +5
Tracing the transition between the diffuse atomic interstellar medium (ISM) and cold, dense gas is crucial for deciphering the star formation cycle in galaxies. Here we present MAC…
Characterizing [C II] Line Emission In Massive Star Forming Clumps
James M. Jackson, David Allingham, Nicholas Killerby-Smith +7
Because the 157.74 micron [C II] line is the dominant coolant of star-forming regions, it is often used to infer the global star-formation rates of galaxies. By characterizing the…
The Interaction Between the Supernova Remnant W41 and the Filamentary Infrared Dark Cloud G23.33-0.30
Taylor G. Hogge, James M. Jackson, David Allingham +6
G23.33-0.30 is a 600 infrared dark molecular filament that exhibits large NH velocity dispersions () and bright, narrow NH(3,3) line…