PROTOPLANETARY DISKS

Formation and evolution of planetary systems

 Coordinatore 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: +44 1392 263744
Fax: +44 1392 263686

 Nazionalità Coordinatore United Kingdom [UK]
 Totale costo 168˙256 €
 EC contributo 168˙256 €
 Programma FP7-PEOPLE
Specific programme "People" implementing the Seventh Framework Programme of the European Community for research, technological development and demonstration activities (2007 to 2013)
 Code Call FP7-PEOPLE-2007-2-1-IEF
 Funding Scheme MC-IEF
 Anno di inizio 2008
 Periodo (anno-mese-giorno) 2008-04-01   -   2010-03-31

 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: Enda
Cognome: Clarke
Email: send email
Telefono: +44 1392 263744
Fax: +44 1392 263686

UK (EXETER) coordinator 0.00

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 Word cloud

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disks    observations   

 Obiettivo del progetto (Objective)

'The goal of this research project is to obtain a global and precise view of protoplanetary disks. To define a consistent line towards this long term objective, the proposal will rely on 1) an extension of multi-wavelengths modelling of disks, on one by hand, by generalizing this kind of studies to an increasing number of disks, on the other hand, by including complementary observations, in particular coming from very large equipments. This step will go through a continuation of the efforts on numerical modelling to 2) take into account radiative transfer in the gas phase of disks (kinematics and abundances). The long term research programme will take part in a willing to develop 3) an approach linking in complementarity observations and modeling of physical processes within disks so as to bring quantitative observational constraints to the models of disk evolution and planet formation.'

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