47 citations · 145 across the 9 of their papers we have counts for
8 papers · 1 filter
CHIMPS2: CO emission in the Central Molecular Zone
S. M. King, T. J. T. Moore, J. D. Henshaw +12
We present the initial data for the () transition of CO obtained from the Central Molecular Zone (CMZ) of the Milky Way as part of the CO Heterodyne Inner Milky…
NEATH III: a molecular line survey of a simulated star-forming cloud
F. D. Priestley, P. C. Clark, S. C. O. Glover +4
We present synthetic line observations of a simulated molecular cloud, utilising a self-consistent treatment of the dynamics and time-dependent chemical evolution. We investigate l…
NH(1-0) as a tracer of dense gas in and between spiral arms
O. Feher, S. E. Ragan, F. D. Priestley +2
Recent advances in identifying giant molecular filaments in galactic surveys allow us to study the interstellar material and its dense, potentially star forming phase on scales com…
The dynamic centres of infrared-dark clouds and the formation of cores
Andrew J. Rigby, Nicolas Peretto, Michael Anderson +7
High-mass stars have an enormous influence on the evolution of the interstellar medium in galaxies, so it is important that we understand how they form. We examine the central clum…
NEATH II: NH as a tracer of imminent star formation in quiescent high-density gas
F. D. Priestley, P. C. Clark, S. C. O. Glover +4
Star formation activity in molecular clouds is often found to be correlated with the amount of material above a column density threshold of . Attempt…
Non-Equilibrium Abundances Treated Holistically (NEATH): the molecular composition of star-forming clouds
F. D. Priestley, P. C. Clark, S. C. O. Glover +4
Much of what we know about molecular clouds, and by extension star formation, comes from molecular line observations. Interpreting these correctly requires knowledge of the underly…