Motivación de un entorno GRID en el área de Astrofísica ( ideas ). Resolución de problemas numéricos complejos en el ámbito de la Astrofísica: Modelos de interacción y evolución galáctica ( sistemas de N cuerpos ) . Modelos Cosmológicos ( Cosmología Numérica)
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The project studies the Compact Groups of Galaxies, where the interactions between galaxies are especially intense, refering to:
The project permit to obtain statistical conclusions about the physics of AGN, combining:
The project will analyse atmospheric pressure/temperature and minor constituents abundances, including non-LTE processes.
The hardware requirements in order to apply Non-LTE inversion technique to work with the high spectral resolution MIPAS measurements are 16 processors and 16 Gbyte shared RAM (min).
The mission will generate alarge amount of data. The analysis will need a
lot of CPU time in order to find oscillation modes and variations in the brightness of the star between 0.01% and 1%.
The sample will have a complete multiwavelength information concerning the ISM, and it will be of special interest to analyse the large amount of data will be generated for high z galaxies.
The data will become public by means of a database. It’ll be integrated in a future Virtual Global Observatory.