LOCALSTAR

Modelling star formation in the local universe

Coordinatore	THE UNIVERSITY OF EXETER    more Spiacenti, non ci sono informazioni su questo coordinatore. Contattare Fabio per maggiori infomrazioni, grazie.
Nazionalità Coordinatore	United Kingdom [UK]
Totale costo	1˙169˙585 €
EC contributo	1˙169˙585 €
Programma	FP7-IDEAS-ERC Specific programme: "Ideas" implementing the Seventh Framework Programme of the European Community for research, technological development and demonstration activities (2007 to 2013)
Code Call	ERC-2011-StG_20101014
Funding Scheme	ERC-SG
Anno di inizio	2011
Periodo (anno-mese-giorno)	2011-11-01   -   2016-10-31

 Partecipanti

#	participant	country	role	EC contrib. [€]
1	THE UNIVERSITY OF EXETER  Organization address address: Northcote House, The Queen's Drive city: EXETER postcode: EX4 4QJ contact info Titolo: Dr. Nome: Clare Cognome: Dobbs Email: send email Telefono: 441393000000 Fax: 441392000000	UK (EXETER)	hostInstitution	1˙169˙585.60
2	THE UNIVERSITY OF EXETER  Organization address address: Northcote House, The Queen's Drive city: EXETER postcode: EX4 4QJ contact info Titolo: Dr. Nome: Enda Cognome: Clarke Email: send email Telefono: 441393000000 Fax: 441392000000	UK (EXETER)	hostInstitution	1˙169˙585.60

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 Obiettivo del progetto (Objective)

'The goal of this proposal is to revolutionize our understanding of star formation in nearby galaxies, using numerical simulations. Traditionally, research in star formation has considered the contraction of a giant molecular cloud (GMC), or more commonly a star forming core, under gravity. However there has been relatively little research on molecular clouds themselves, even though they provide the initial conditions for star formation, and thus determine the main assumptions for theories of star formation. The proposed research will focus on the scales of giant molecular clouds, the clouds of molecular hydrogen (H2) where most star formation takes place in nearby galaxies. These objects link galactic scale physics with the small scale physics of star formation. Only now are the computational resources becoming available to study the interstellar medium (ISM) numerically on galactic scales, and model the complex processes involved in GMC and star formation. Simultaneously observational programs (e.g. ALMA, Herschel, CARMA) are starting to resolve GMCs in nearby galaxies. Our research will involve performing calculations on scales from individual GMCs to interacting galaxies, and comparing to forthcoming observations to answer some of the most fundamental questions in star formation, such as why star formation is inefficient, how do GMCs form and what are their lifetimes.'