Search Results - "GLOVER, S"
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Uncertainties in H2 and HD chemistry and cooling and their role in early structure formation
Published in Monthly notices of the Royal Astronomical Society (01-08-2008)“…At low temperatures, the main coolant in primordial gas is molecular hydrogen, H2. Recent work has shown that primordial gas that is not collapsing…”
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The SILCC (SImulating the LifeCycle of molecular Clouds) project – I. Chemical evolution of the supernova-driven ISM
Published in Monthly notices of the Royal Astronomical Society (21-11-2015)“…The SILCC (SImulating the Life-Cycle of molecular Clouds) project aims to self-consistently understand the small-scale structure of the interstellar medium…”
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SILCC-Zoom: the dynamic and chemical evolution of molecular clouds
Published in Monthly notices of the Royal Astronomical Society (21-12-2017)“…Abstract We present 3D ‘zoom-in’ simulations of the formation of two molecular clouds out of the galactic interstellar medium. We model the clouds – identified…”
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On the relationship between molecular hydrogen and carbon monoxide abundances in molecular clouds
Published in Monthly notices of the Royal Astronomical Society (01-03-2011)“…The most usual tracer of molecular gas is line emission from CO. However, the reliability of this tracer has long been questioned in environments different…”
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The density variance-Mach number relation in supersonic turbulence - I. Isothermal, magnetized gas
Published in Monthly notices of the Royal Astronomical Society (01-07-2012)“…It is widely accepted that supersonic, magnetized turbulence plays a fundamental role for star formation in molecular clouds. It produces the initial dense gas…”
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Mapping Metallicity Variations across Nearby Galaxy Disks
Published in The Astrophysical journal (10-12-2019)“…The distribution of metals within a galaxy traces the baryon cycle and the buildup of galactic disks, but the detailed gas phase metallicity distribution…”
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Fervent: chemistry-coupled, ionizing and non-ionizing radiative feedback in hydrodynamical simulations
Published in Monthly notices of the Royal Astronomical Society (21-11-2015)“…We introduce a radiative transfer code module for the magnetohydrodynamical adaptive mesh refinement code flash 4. It is coupled to an efficient chemical…”
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Characterizing the mucin-degrading capacity of the human gut microbiota
Published in Scientific reports (19-05-2022)“…Mucin-degrading microbes are known to harbor glycosyl hydrolases (GHs) which cleave specific glycan linkages. Although several microbial species have been…”
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The PHANGS–MUSE nebular catalogue
Published in Monthly notices of the Royal Astronomical Society (22-02-2023)“…ABSTRACT Ionized nebulae provide critical insights into the conditions of the interstellar medium (ISM). Their bright emission lines enable the measurement of…”
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Dense molecular gas properties on 100 pc scales across the disc of NGC 3627
Published in Monthly notices of the Royal Astronomical Society (01-09-2021)“…It is still poorly constrained how the densest phase of the interstellar medium varies across galactic environment. A large observing time is required to…”
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WARPFIELD-EMP: The self-consistent prediction of emission lines from evolving H ii regions in dense molecular clouds
Published in Monthly notices of the Royal Astronomical Society (21-07-2020)“…ABSTRACT We present the warpfield emission predictor, warpfield-emp, which couples the 1D stellar feedback code warpfield with the cloudy H iiregion/PDR code…”
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The Molecular Gas Reservoirs of z ∼ 2 Galaxies: A Comparison of CO(1−0) and Dust-based Molecular Gas Masses
Published in The Astrophysical journal (20-07-2019)“…We test the use of long-wavelength dust continuum emission as a molecular gas tracer at high redshift, via a unique sample of a dozen z ∼ 2 galaxies with…”
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Modelling the supernova-driven ISM in different environments
Published in Monthly notices of the Royal Astronomical Society (01-05-2015)“…We use hydrodynamical simulations in a (256 pc)3 periodic box to model the impact of supernova (SN) explosions on the multiphase interstellar medium (ISM) for…”
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Modelling CO formation in the turbulent interstellar medium
Published in Monthly notices of the Royal Astronomical Society (01-05-2010)“…We present results from high-resolution three-dimensional simulations of turbulent interstellar gas that self-consistently follow its coupled thermal, chemical…”
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On the resolution requirements for modelling molecular gas formation in solar neighbourhood conditions
Published in Monthly notices of the Royal Astronomical Society (01-04-2019)Get full text
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LEGO – II. A 3 mm molecular line study covering 100 pc of one of the most actively star-forming portions within the Milky Way disc
Published in Monthly notices of the Royal Astronomical Society (11-09-2020)“…ABSTRACT The current generation of (sub)mm-telescopes has allowed molecular line emission to become a major tool for studying the physical, kinematic, and…”
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On the detection of supermassive primordial stars – II. Blue supergiants
Published in Monthly notices of the Royal Astronomical Society (21-09-2019)“…ABSTRACT Supermassive primordial stars in hot, atomically cooling haloes at z ∼ 15–20 may have given birth to the first quasars in the Universe. Most…”
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Electron-Transfer/Higher-Energy Collision Dissociation (EThcD)-Enabled Intact Glycopeptide/Glycoproteome Characterization
Published in Journal of the American Society for Mass Spectrometry (01-09-2017)“…Protein glycosylation, one of the most heterogeneous post-translational modifications, can play a major role in cellular signal transduction and disease…”
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Comparing the pre-SNe feedback and environmental pressures for 6000 H ii regions across 19 nearby spiral galaxies
Published in Monthly notices of the Royal Astronomical Society (28-10-2021)“…ABSTRACT The feedback from young stars (i.e. pre-supernova) is thought to play a crucial role in molecular cloud destruction. In this paper, we assess the…”
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Population III X-ray binaries and their impact on the early universe
Published in Monthly notices of the Royal Astronomical Society (01-05-2023)“…ABSTRACT The first population of X-ray binaries (XRBs) is expected to affect the thermal and ionization states of the gas in the early Universe. Although these…”
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