2 citations · 3 across the 10 of their papers we have counts for
10 papers
UCLCHEM 4.0: An open source gas-grain astrochemistry simulation framework
Gijs Vermariën, Serena Viti, Tobias M. Dijkhuis +4
Astrochemical modelling is a key tool for interpreting the formation and destruction of molecules in the interstellar medium, complementing the increasingly detailed observations e…
BISTRO Survey: Gravity-Dominated and Magnetically Regulated Star Formation in M17 SW
Mengke Zhao, Keping Qiu, Ji-hyun Kang +27
We present high-resolution magnetic field maps of the M17 SW molecular cloud using JCMT 850 m dust polarization at a scale of 14. The magnetic field exhibits a distinct arc-…
The Impact of Radiation Environment on the Evolution and Fragmentation of Protostellar Discs
Matt T. Cusack, Paul C. Clark, Ken Rice +5
We present high-resolution zoom-in simulations of molecular clouds exposed to an interstellar radiation field and cosmic ray ionisation rate up to 1000 times stronger than that of…
NEATH V: the relationship between line emission from dense gas tracers and the star formation rate
F. D. Priestley, P. C. Clark, S. C. O. Glover +5
The Gao-Solomon relationship between the luminosity of the HCN line and the star formation rate (SFR) is observed to remain close to linear over scales ranging from individ…
Assessing Self-Absorbed Molecular Lines as Tracers of Gravitational Collapse
Lillian Y. Cai, Felix D. Priestley, Sarah E. Ragan
Red-shifted self-absorption features in molecular lines are commonly interpreted as signatures of gravitational collapse in pre- and protostellar cores. The shape of the line profi…
Dense gas tracers in and between spiral arms: from Giant Molecular Filaments to star-forming clumps
O. Feher, S. E. Ragan, F. D. Priestley +1
Giant Molecular Filaments are opportune locations in our Galaxy to study the star-forming interstellar matter and its accumulation on spatial scales comparable to those now becomin…
NEATH IV: an early onset of complex organic chemistry in molecular clouds
F. D. Priestley, P. C. Clark, S. E. Ragan +6
Complex organic molecules (COMs) are widely detected in protostellar and protoplanetary systems, where they are thought to have been inherited in large part from earlier evolutiona…
The fragmentation of molecular clouds in starburst environments
Matt T. Cusack, Paul C. Clark, Simon C. O. Glover +4
A significant amount of star formation occurs and has occurred in environments unlike the solar neighbourhood. The majority of stars formed closer to the peak of the cosmic star fo…
Cloud Collision Signatures in the Central Molecular Zone
Rees A. Barnes, Felix D. Priestley
Molecular cloud collisions are a prominent theory for the formation of stars. Observational studies into cloud collisions identify the collision via a bridging feature: a continuou…
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…