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.
Organisations
Publications
Owen J
(2010)
Radiation-hydrodynamic models of X-ray and EUV photoevaporating protoplanetary discs
in Monthly Notices of the Royal Astronomical Society
Rothman L
(2010)
HITEMP, the high-temperature molecular spectroscopic database
in Journal of Quantitative Spectroscopy and Radiative Transfer
Royer P
(2010)
PACS and SPIRE spectroscopy of the red supergiant VY CMa
in Astronomy and Astrophysics
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
Tennyson J
(2010)
IUPAC critical evaluation of the rotational-vibrational spectra of water vapor. Part II
in Journal of Quantitative Spectroscopy and Radiative Transfer
Urru A
(2010)
Ro-vibrational spectra of C 2 H 2 based on variational nuclear motion calculations
in Molecular Physics
Wesson R
(2010)
The destruction and survival of dust in the shell around SN 2008S
in Monthly Notices of the Royal Astronomical Society
Yurchenko SN
(2009)
A variationally computed T = 300 K line list for NH3.
in The journal of physical chemistry. A