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The MIRACLE Consortium: Modelling the Universe - From Atomic to Large Scales Structures

Lead Research Organisation: UNIVERSITY COLLEGE LONDON
Department Name: Physics and Astronomy

Abstract

The MIRACLE High Performance Computing supports high-end computing in astrophysics, covering the following projects: * the optical properties of small molecules; * 3D radiative (magneto)-hydro-dynamical simulations of stellar formation, * stellar structure and evolution; * astrochemical simulations in 3D physical simulations, especially the polymerization of astrophysical dust particles; * catalytic and optical properties of astronomical dust candidates; * 3D spectral line and continuum radiative transfer; * 3D simulations of planetary atmospheres and extra-solar planetary atmospheres and * full hydro-dynamical simulation of the intra-cluster medium.

Publications

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Tennyson J (2010) IUPAC critical evaluation of the rotational-vibrational spectra of water vapor. Part II in Journal of Quantitative Spectroscopy and Radiative Transfer

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Beaulieu J (2010) Water in the atmosphere of HD 209458b from 3.6-8 µm IRAC photometric observations in primary transit Water in the atmosphere of HD 209458b in Monthly Notices of the Royal Astronomical Society

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Császár A (2010) First-principles prediction and partial characterization of the vibrational states of water up to dissociation in Journal of Quantitative Spectroscopy and Radiative Transfer

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Royer P (2010) PACS and SPIRE spectroscopy of the red supergiant VY CMa in Astronomy and Astrophysics

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Sochi T (2010) A computed line list for the H2D+ molecular ion A computed line list for the H2D+ molecular ion in Monthly Notices of the Royal Astronomical Society

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Decin L (2010) Silicon in the dust formation zone of IRC +10216 in Astronomy and Astrophysics

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Achilleos N (2010) A model of force balance in Saturn's magnetodisc in Monthly Notices of the Royal Astronomical Society

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Ercolano B (2011) The clearing of discs around late-type T Tauri stars: constraints from the infrared two-colour plane Disc clearing in M stars in Monthly Notices of the Royal Astronomical Society