DA
David M. Acreman
astro-ph.SRastro-ph.GAastro-ph.EPastro-phastro-ph.IMphysics.ao-phphysics.flu-dyn
On Valency
published · living versionsW_nyrwa6jm·v1 · currentpublished
Accuracy tests of radiation schemes used in hot Jupiter global circulation models
with David Skålid Amundsen, Isabelle Baraffe, Pascal Tremblin, James Manners +2
1 version
Preprints & journals
30 papers in the corpus · 2003–2019Synthetic molecular line observations of the first hydrostatic core from chemical calculations1906.01324v1 · Alison K. Young, Matthew R. Bate, Tim J. Harries et al.2019 · 13 citationsarXiv
The TORUS radiation transfer code1903.06672v1 · Tim Harries, Tom Haworth, David Acreman et al.2019 · 62 citationsarXiv
Simultaneous spectral energy distribution and near-infrared interferometry modeling of HD 1426661808.10762v1 · Claire L Davies, Stefan Kraus, Tim J Harries et al.2018 · 20 citationsarXiv
Exonephology: Transmission spectra from a 3D simulated cloudy atmosphere of HD209458b1808.05887v1 · S. Lines, J. Manners, N. J. Mayne et al.2018 · 64 citationsarXiv
Simulating the cloudy atmospheres of HD 209458 b and HD 189733 b with the 3D Met Office Unified Model1803.00226v1 · S. Lines, N. J. Mayne, Ian A. Boutle et al.2018 · 109 citationsA&A 615, A97 (2018)
The effect of metallicity on the atmospheres of exoplanets with fully coupled 3D hydrodynamics, equilibrium chemistry, and radiative transfer1801.01045v1 · Benjamin Drummond, N. J. Mayne, Isabelle Baraffe et al.2018 · 65 citationsarXiv
Results from a set of three-dimensional numerical experiments of a hot Jupiter atmosphere1704.00539v1 · N. J. Mayne, F. Debras, I. Baraffe et al.2017 · 70 citationsA&A 604, A79 (2017)
Exploring the climate of Proxima B with the Met Office Unified Model1702.08463v2 · Ian A. Boutle, Nathan J. Mayne, Benjamin Drummond et al.2017 · 131 citationsA&A 601, A120 (2017)
The mineral clouds on HD 209458b and HD189733b1603.04022v4 · Ch. Helling, G. Lee, I. Dobbs-Dixon et al.2016 · 98 citationsarXiv
Modelling multi-wavelength observational characteristics of bow shocks from runaway early type stars1511.03059v1 · David M. Acreman, Ian R. Stevens, Tim J. Harries2015 · 21 citationsarXiv
On the relative importance of different microphysics on the D-type expansion of galactic HII regions1508.00900v1 · Thomas J. Haworth, Tim J. Harries, David M. Acreman et al.2015 · 33 citationsarXiv
The morphology of the Milky Way - II. Reconstructing CO maps from disc galaxies with live stellar distributions1503.05563v1 · Alex R. Pettitt, Clare L. Dobbs, David M. Acreman et al.2015 · 49 citationsarXiv
Synthetic CO, H2 and HI surveys of the Galactic 2nd Quadrant, and the properties of molecular gas1412.2785v1 · A. Duarte-Cabral, D. M. Acreman, C. L. Dobbs et al.2014 · 34 citationsarXiv
The morphology of the Milky Way - I. Reconstructing CO maps from simulations in fixed potentials1406.4150v1 · Alex R. Pettitt, Clare L. Dobbs, David M. Acreman et al.2014 · 67 citationsarXiv
Accuracy tests of radiation schemes used in hot Jupiter global circulation models1402.0814v2 · David Sk\aalid Amundsen, Isabelle Baraffe, Pascal Tremblin et al.2014 · 182 citationsarXivon Valency
The UM, a fully--compressible, non--hydrostatic, deep atmosphere GCM, applied to hot Jupiters1311.2083v1 · N. J. Mayne, I. Baraffe, David M. Acreman et al.2013 · 0 citationsarXiv
Using the UM dynamical cores to reproduce idealised 3D flows1310.6041v1 · N. J. Mayne, I. Baraffe, David M. Acreman et al.2013 · 75 citationsarXiv
Assessing molecular line diagnostics of triggered star formation using synthetic observations1303.1322v2 · Thomas J. Haworth, Tim J. Harries, David M. Acreman et al.2013 · 19 citationsarXiv
Radiation hydrodynamics simulations of massive star formation using Monte Carlo radiation transfer1209.1512v1 · Tim J. Harries, Tom J. Haworth, David Acreman2012 · 5 citationsarXiv
Testing models of triggered star formation: theory and observation1208.1704v2 · Thomas J. Haworth, Tim J. Harries, David M. Acreman2012 · 1 citationarXiv
Testing diagnostics of triggered star formation1205.6993v2 · Thomas J. Haworth, Tim J. Harries, David M. Acreman2012 · 20 citationsarXiv
Bayesian fitting of Taurus brown dwarf spectral energy distributions1203.6657v1 · N. J. Mayne, Tim J. Harries, John Rowe et al.2012 · 14 citationsarXiv
The structure of HI in galactic disks: Simulations vs observations1201.4970v1 · David M. Acreman, Clare L. Dobbs, Christopher M. Brunt et al.2012 · 13 citationsarXiv
Three-dimensional molecular line transfer: A simulated star-forming region1005.1648v1 · David Rundle, Tim J. Harries, David M. Acreman et al.2010 · 37 citationsarXiv
A Synthetic 21-cm Galactic Plane Survey of an SPH Galaxy Simulation1004.4096v1 · Kevin A. Douglas, David M. Acreman, Clare L. Dobbs et al.2010 · 16 citationsMNRAS 407 (2010) 405-414
Synthetic HI observations of a simulated spiral galaxy1004.3204v1 · David M. Acreman, Kevin A. Douglas, Clare L. Dobbs et al.2010 · 13 citationsarXiv
Modelling circumstellar discs with 3D radiation hydrodynamics0912.2030v1 · David M. Acreman, Tim J. Harries, David A. Rundle2009 · 23 citationsarXiv
Synthetic Observations of the HI Line in SPH-Simulated Spiral Galaxies0909.0187v1 · Kevin A. Douglas, David Acreman, Clare Dobbs et al.2009 · 0 citationsarXiv
The cool wake around 4C 34.16 as seen by XMM-Newtonastro-ph/0504420v1 · I. Sakelliou, D.M. Acreman, M.J. Hardcastle et al.2005 · 15 citationsMon.Not.Roy.Astron.Soc. 360 (2005) 1063-1068
Simulations of the Effects of Stripping and Accretion on Galaxy Haloes in Clustersastro-ph/0302322v1 · David M. Acreman, Ian R. Stevens, Trevor J. Ponman et al.2003 · 59 citationsMon.Not.Roy.Astron.Soc. 341 (2003) 1333
Career total: 51 works. 30 are in this corpus.
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