Search Results - "Acreman, D. M."

On the relative importance of different microphysics on the D-type expansion of galactic H ii regions by Haworth, T. J., Harries, T. J., Acreman, D. M., Bisbas, T. G.

“…Radiation hydrodynamics (RHD) simulations are used to study many astrophysical phenomena; however, they require the use of simplified radiation transport and…”
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Using the UM dynamical cores to reproduce idealised 3-D flows by Mayne, N. J, Baraffe, I, Acreman, D. M, Smith, C, Wood, N, Amundsen, D. S, Thuburn, J, Jackson, D. R

“…We demonstrate that both the current (New Dynamics), and next generation (ENDGame) dynamical cores of the UK Met Office global circulation model, the UM,…”
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Exonephology: transmission spectra from a 3D simulated cloudy atmosphere of HD 209458b by Lines, S, Manners, J, Mayne, N J, Goyal, J, Carter, A L, Boutle, I A, Lee, Elspeth, Helling, Ch, Drummond, B, Acreman, D M, Sing, D K

“…ABSTRACT We present high-resolution transmission spectra, calculated directly from a 3D radiative hydrodynamic simulation that includes kinetic cloud…”
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Simulations of the effects of stripping and accretion on galaxy haloes in clusters by Acreman, David M., Stevens, Ian R., Ponman, Trevor J., Sakelliou, Irini

“…We present results from a series of hydrodynamic simulations investigating ram pressure stripping of galactic haloes as the host galaxy falls radially into a…”
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The cool wake around 4C 34.16 as seen by XMM-Newton by Sakelliou, I., Acreman, D. M., Hardcastle, M. J., Merrifield, M. R., Ponman, T. J., Stevens, I. R.

“…We present XMM-Newton observations of the wake—radio galaxy system 4C 34.16, which shows a cool and dense wake trailing behind the host galaxy of 4C 34.16. A…”
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Synthetic CO, H2 and H i surveys of the second galactic quadrant, and the properties of molecular gas by Duarte-Cabral, A., Acreman, D. M., Dobbs, C. L., Mottram, J. C., Gibson, S. J., Brunt, C. M., Douglas, K. A.

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The use of Argo for validation and tuning of mixed layer models by Acreman, D.M., Jeffery, C.D.

“…We present results from validation and tuning of 1-D ocean mixed layer models using data from Argo floats and data from Ocean Weather Station Papa (145°W,…”
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Galaxies in clusters: the observational characteristics of bow shocks, wakes and tails by Stevens, Ian R., Acreman, David M., Ponman, Trevor J.

“…The dynamical signatures of the interaction between galaxies in clusters and the intracluster medium (ICM) can potentially yield significant information about…”
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Exonephology: Transmission spectra from a 3D simulated cloudy atmosphere of HD209458b by Lines, S, Manners, J, Mayne, N. J, Goyal, J, Carter, A. L, Boutle, I. A, Lee, E. K. H, Helling, Ch, Drummond, B, Acreman, D. M, Sing, D. K

“…We present high resolution transmission spectra, calculated directly from a 3D radiative-hydrodynamics simulation that includes kinetic cloud formation, for…”
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Synthetic CO, H2 and HI surveys of the Galactic 2nd Quadrant, and the properties of molecular gas by Duarte-Cabral, A, Acreman, D. M, Dobbs, C. L, Mottram, J. C, Gibson, S. J, Brunt, C. M, Douglas, K. A

“…We present CO, H2, HI and HISA distributions from a set of simulations of grand design spirals including stellar feedback, self-gravity, heating and cooling…”
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Synthetic CO, H sub( 2) and H I surveys of the second galactic quadrant, and the properties of molecular gas by Duarte-Cabral, A, Acreman, D M, Dobbs, C L, Mottram, J C, Gibson, S J, Brunt, C M, Douglas, K A

“…We present CO, H..., H i and HISA (H i self-absorption) distributions from a set of simulations of grand design spirals including stellar feedback,…”
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Synthetic CO, H^sub 2^ and H I surveys of the second galactic quadrant, and the properties of molecular gas by Duarte-Cabral, A, Acreman, D M, Dobbs, C L, Mottram, J C, Gibson, S J, Brunt, C M, Douglas, K A

“…We present CO, H..., H i and HISA (H i self-absorption) distributions from a set of simulations of grand design spirals including stellar feedback,…”
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The cool wake around 4C 34.16 as seen by XMM-Newton by Sakelliou, I., Acreman, D. M., Hardcastle, M. J., Merrifield, M. R., Ponman, T. J., Stevens, I. R.

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The cool wake around 4C 34.16 as seen by XMM-Newton by Sakelliou, I, Acreman, D. M, Hardcastle, M. J, Merrifield, M. R, Ponman, T. J, Stevens, I. R

“…Mon.Not.Roy.Astron.Soc. 360 (2005) 1063-1068 We present XMM-Newton observations of the wake-radiogalaxy system 4C34.16, which shows a cool and dense wake…”
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