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Financement de l’UE (639 400 €) : Poussière et gaz dans les disques formant des planètes Hor13/11/2018 Programme de recherche et d'innovation de l'UE « Horizon »
Texte
Poussière et gaz dans les disques formant des planètes
Planet formation is a widespread by-product of the process of star formation itself and occurs within relatively thin and dense protostellar discs made of gas and dust that orbit the newborn star. Such discs can now be probed with unprecedented detail thanks to high resolution telescopes and instruments, such as the Atacama Large Millimeter Array (ALMA) at sub-millimeter wavelegths or the SPHERE instrument at the Very large telescope (VLT) in the near infrared, which are both capable of probing nearby star formation regions with a spatial resolution of a few astronomical units. The overall aim of this project is to to strengthen the collaboration of groups located in Europe, USA, Chile and Australia - many of them already collaborating actively - in order to (1) develop and use suitable numerical algorithms and techniques to address key unsolved issues related to the interaction of newborn planets with the gas and dust environment in which they are born and (2) to compare such models with the most advanced observations of protostellar discs, obtained with high resolution telescopes in the IR and sub-mm.
https://cordis.europa.eu/project/id/823823
Cette annonce se réfère à une date antérieure et ne reflète pas nécessairement l’état actuel. L’état actuel est présenté à la page suivante : ARIZONA BOARD OF REGENTS, Tempe, États-Unis.
