42 citations · 87 across the 9 of their papers we have counts for
9 papers
CHIMPS2: The physical properties and star formation efficiency of molecular gas in the Central Molecular Zone
S. M. King, T. J. T. Moore, S. N. Longmore +4
We present Local Thermodynamic Equilibrium (LTE) estimates of the physical properties and star formation efficiency (SFE) of molecular gas in the Central Molecular Zone (CMZ), usin…
MAJORS II: HCO+& HCN Abundances in W40
René Plume, David J. Eden, Malcolm J. Currie +34
We present observations of HCN and HCO J = in the central region of the W40 massive star forming region. The observations were taken as part of a p…
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…
The impact of shear on the rotation of Galactic plane molecular clouds
Raffaele Rani, Jia-Lun Li, Toby J. T. Moore +4
Stars form in the densest regions of molecular clouds, however, there is no universal understanding of the factors that regulate cloud dynamics and their influence on the gas-to-st…
Identification of molecular clouds in emission maps: a comparison between methods in the \ce{^{13}CO}/\ce{C^{18}O} () Heterodyne Inner Milky Way Plane Survey
Raffaele Rani, Toby J. T. Moore, David J. Eden +3
The growing range of automated algorithms for the identification of molecular clouds and clumps in large observational datasets has prompted the need for the direct comparison of t…
Solenoidal turbulent modes and star formation efficiency in Galactic-plane molecular clouds
Raffaele Rani, Toby J. T. Moore, David J. Eden +1
It is speculated that the high star-formation efficiency observed in spiral-arm molecular clouds is linked to the prevalence of compressive (curl-free) turbulent modes, while the s…
CHIMPS2: Survey description and CO emission in the Galactic Centre
D. J. Eden, T. J. T. Moore, M. J. Currie +103
The latest generation of Galactic-plane surveys is enhancing our ability to study the effects of galactic environment upon the process of star formation. We present the first data…
Compact galaxies and the size-mass galaxy distribution from a colour-selected sample at 0.04 < z < 0.15 supplemented by ugrizYJHK photometric redshifts
Ivan K. Baldry, Tricia Sullivan, Raffaele Rani +1
The size-mass galaxy distribution is a key diagnostic for galaxy evolution. Massive compact galaxies are potential surviving relics of a high-redshift phase of star formation. Some…
Characteristic scale of star formation. I. Clump formation efficiency on local scales
D. J. Eden, T. J. T. Moore, R. Plume +12
We have used the ratio of column densities (CDR) derived independently from the 850-m continuum JCMT Plane Survey (JPS) and the CO/CO Heterodyne Inner Mi…