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ICYBOB SIGNED

Initial Conditions of YMCs, Birth of OB associations and long term evolution of stellar clusters

Total Cost €

EC-Contrib. €

Partnership

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ICYBOB project word cloud

Explore the words cloud of the ICYBOB project. It provides you a very rough idea of what is the project "ICYBOB" about.

astronomy numericists scales star stages gas isolated pioneers theoretical simulations gmcs numerically causes cloud stellar galaxy gaiaaia date galactic questions life galaxies transform numerical ob first follow fundamental pi destruction survive ymcs cluster evolve something clouds clusters realistic instrument counterpart happens attempted performing perform molecular disperse evolution clustersgiant associations gmc orbit era ivii sophisticated form

Project "ICYBOB" data sheet

The following table provides information about the project.

Coordinator	THE UNIVERSITY OF EXETER Organization address address: THE QUEEN'S DRIVE NORTHCOTE HOUSE city: EXETER postcode: EX4 4QJ website: www.ex.ac.uk contact info title: n.a. name: n.a. surname: n.a. function: n.a. email: n.a. telephone: n.a. fax: n.a.
Coordinator Country	United Kingdom [UK]
Total cost	1˙980˙385 €
EC max contribution	1˙980˙385 € (100%)
Programme	1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
Code Call	ERC-2018-COG
Funding Scheme	ERC-COG
Starting year	2019
Duration (year-month-day)	from 2019-06-01 to 2024-05-31

Partnership

Take a look of project's partnership.

#	participants	country	role	EC contrib. [€]
1	THE UNIVERSITY OF EXETER THE UNIVERSITY OF EXETER Organization address address: THE QUEEN'S DRIVE NORTHCOTE HOUSE city: EXETER postcode: EX4 4QJ website: www.ex.ac.uk contact info title: n.a. name: n.a. surname: n.a. function: n.a. email: n.a. telephone: n.a. fax: n.a.	UK (EXETER)	coordinator	1˙980˙385.00

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Project objective

The goal of this proposal is to establish a new era of stellar cluster evolution research by performing numerical simulations on different scales, and of different stages of a cluster’s life, from the formation of YMCs, the formation and evolution of OB associations, to the evolution of clusters and associations in galaxies. The PI is one of the pioneers of galactic simulations of GMC and star formation was one of the first numericists to perform galactic scale simulations of molecular cloud formation and evolution, and has produced some of the most realistic and sophisticated isolated simulations of galaxies in this field to date. The next challenge is to follow cluster evolution, something which has not yet been attempted numerically. And, with the GaiaAIA instrument set to transform stellar astronomy in our Galaxy, our work will provide a fundamental theoretical counterpart. Key questions we will address include i) how does gas disperse from new clusters and what happens to that gas, ii) how do YMCs form, iii) how do new clustersGiant Molecular Clouds (GMCs) evolve into OB associations, and ivii) how long can clusters survive for as they orbit a galaxy and what causes their destruction.

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The information about "ICYBOB" are provided by the European Opendata Portal: CORDIS opendata.