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Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 04/2012, Volume 421, Issue 4, pp. 3217 - 3221
  The formation of stars is a key process in the early universe with far-reaching consequences for further cosmic evolution. While stars forming from truly... 
Stars: abundances | Stars: Population II | Stars: Population III | Stars: formation | Stars: luminosity function, mass function | Early Universe | Thermodynamics | Astrophysics | Star & galaxy formation | Stars & galaxies | Metals | Origins | Dust | Cooling | Metallicity | Stars | Continuums | Universe | Sun | Fragmentation
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 07/2016, Volume 460, Issue 1, pp. 82 - 102
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 11/2019
Abstract We present a suite of high resolution radiation hydrodynamic simulations of a small patch (1 kpc2) of the inter-stellar medium (ISM) performed with... 
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 10/2019
Abstract Jets from young stellar objects provide insight into the workings of the beating heart at the centre of star forming cores. In some cases, multiple... 
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 02/2020, Volume 492, Issue 2, pp. 1594 - 1613
ABSTRACT We introduce a new suite of simulations, ‘The Cloud Factory’, which self-consistently forms molecular cloud complexes at high enough resolution to... 
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 02/2020, Volume 492, Issue 2, pp. 2973 - 2995
ABSTRACT We present here the first of a series of papers aimed at better understanding the evolution and properties of giant molecular clouds (GMCs) in a... 
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 11/2015, Volume 453, Issue 3, p. 2901
  We investigate how uncertainties in the chemical and cooling rate coefficients relevant for a metal-free gas influence our ability to determine the critical... 
Black holes | Hydrogen | Chemical reactions | Star & galaxy formation | Astronomy
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2016, Volume 456, Issue 4, p. 3596
  Carbon monoxide (CO) is widely used as a tracer of molecular hydrogen (H^sub 2^) in metal-rich galaxies, but is known to become ineffective in... 
Molecules | Gases | Stars & galaxies | Metals | Carbon monoxide | Astronomy
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2016, Volume 456, Issue 4, pp. 3596 - 3596
Carbon monoxide (CO) is widely used as a tracer of molecular hydrogen (H sub( 2)) in metal-rich galaxies, but is known to become ineffective in low-metallicity... 
Clouds | Computer simulation | Star formation | Metallicity | Mathematical models | Carbon monoxide | Carbon | Tracers
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 08/2015, Volume 451, Issue 2, pp. 2082 - 2082
The direct collapse model for the formation of massive seed black holes in the early Universe attempts to explain the observed number density of supermassive... 
Collapse | Seeds | Cooling | Chemical reactions | Black holes (astronomy) | Universe | Formations | Density
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 08/2015, Volume 451, Issue 2, p. 2082
  The direct collapse model for the formation of massive seed black holes in the early Universe attempts to explain the observed number density of supermassive... 
Cooling | Simulation | Black holes | Universe | Chemical reactions | Star & galaxy formation | Astronomy
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 02/2019, Volume 483, Issue 2, pp. 2547 - 2560
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 04/2015, Volume 448, Issue 2, p. 1607
  We use detailed numerical simulations of a turbulent molecular cloud to study the usefulness of the [C I] 609 and 370 μm fine structure emission lines as... 
Temperature | Clouds | Density | Carbon | Astronomy | Emissions
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 01/2015, Volume 453, Issue 3, pp. 2901 - 2901
We investigate how uncertainties in the chemical and cooling rate coefficients relevant for a metal-free gas influence our ability to determine the critical... 
Collapse | Field strength | Uncertainty | Seeds | Cooling rate | Black holes (astronomy) | Ultraviolet | Coefficients
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 11/2016, Volume 462, Issue 4, pp. 3591 - 3601
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 04/2012, Volume 421, Issue 3, pp. 2531 - 2542
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 04/2017, Volume 466, Issue 1, p. 407
  Hydrodynamical simulations of star formation often do not possess the dynamic range needed to fully resolve the build-up of individual stars and star... 
Simulation | Supernovae | Accretion disks | Star & galaxy formation | Astronomy
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 04/2017, Volume 466, Issue 1, pp. 407 - 407
Hydrodynamical simulations of star formation often do not possess the dynamic range needed to fully resolve the build-up of individual stars and star clusters,... 
Stellar mass | Stars | Samples | Astronomical models | Mathematical models | Statistical methods | Star clusters | Accumulation
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 02/2017, Volume 465, Issue 2, p. 2277
  The carbon monoxide (CO) rotational transition lines are the most common tracers of molecular gas within giant molecular clouds (MCs). We study the ratio... 
Fluid mechanics | Simulation | Carbon monoxide | Physical properties | Star & galaxy formation
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 02/2017, Volume 465, Issue 2, pp. 2277 - 2277
The carbon monoxide (CO) rotational transition lines are the most common tracers of molecular gas within giant molecular clouds (MCs). We study the ratio... 
Clouds | Molecular clouds | Emission analysis | Carbon monoxide | Excitation | Physical properties | Conversion | Tracers
Journal Article
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