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Editions Universitaires Europeennes Etude de la dynamique collisionnelle des molécules N2H+ et H2O:: implication sur la caractérisation des régions de formation d'étoiles

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Description
La compréhension des processus amenant à la formation d'étoiles depuis la phase dense du milieu interstellaire est possible via l'observation des molécules. Celles-ci nous permettent de contraindre, par l'intermédiaire d'une modélisation de leur émission, les conditions physiques, dynamiques et chimiques présentes dans les nuages au cours des différents stades de l'effondrement. Les milieux sondés lors de ce type d'étude correspondent, pour la plupart des molécules, à des conditions pour lesquelles le peuplement des niveaux d'énergie s'effectue hors équilibre thermodynamique. L'analyse du rayonnement nécessite alors des données de physique microscopique dont la précision influence fortement la description des régions modélisées. C'est dans ce contexte que s'inscrit le présent ouvrage, où sont détaillés d'une part les méthodes de dynamique quantique permettant le calcul de taux de collisions entre molécules et d'autre part, la manière dont ces données sont ensuite utilisées afin de reproduire les observations du Milieu Interstellaire.

Product Specifications
Brand
Editions Universitaires Europeennes
Format
paperback
ASIN
6131509077
Category
Books > Subjects > Science, Nature & Maths > Astronomy & Space Science > Astronomy
Domain
Amazon UK
Release Date
15 October 2010
Listed Since
18 October 2010

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