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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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Guio P (2009) The VOISE algorithm: a versatile tool for automatic segmentation of astronomical images in Monthly Notices of the Royal Astronomical Society

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Grechko M (2009) State-selective spectroscopy of water up to its first dissociation limit. in The Journal of chemical physics

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Barber R (2009) Water in the near-infrared spectrum of comet 8P/Tuttle in Monthly Notices of the Royal Astronomical Society

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Ercolano B (2009) Gas phase diagnostics of protoplanetary disc extension in Astronomy & Astrophysics

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Bastian N (2009) Hierarchical star formation in M33: properties of the star-forming regions in Astrophysics and Space Science

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Yurchenko SN (2009) A variationally computed T = 300 K line list for NH3. in The journal of physical chemistry. A

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Ercolano B (2010) Metallicity, planet formation and disc lifetimes in Monthly Notices of the Royal Astronomical Society