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EU funding (€639,400): Dust and gas in planet forming discs Hor13 Nov 2018 EU Research and Innovation programme "Horizon"

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Dust and gas in planet forming discs

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.


Funded Companies:

Company name Funding amount
ARIZONA BOARD OF REGENTS ?
Ecole Normale Superieure de Lyon €105,800
EUROPEAN SOUTHERN OBSERVATORY - ESO EUROPEAN ORGANISATION FOR ASTRONOMICAL RESEARCH IN THE SOUTHERN HEMISPHERE €138,000
The Chancellor Masters and Scholars of the University of Cambridge €87,400
Universita Degli Studi Di Milano €174,800
University of Leeds €54,280
University of Leicester €79,120

Source: https://cordis.europa.eu/project/id/823823

The filing refers to a past date, and does not necessarily reflect the current state. The current state is available on the following page: ARIZONA BOARD OF REGENTS, Tempe, United States.

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