Notes - Instituto de AstrofÃsica de AndalucÃa
Notes - Instituto de AstrofÃsica de AndalucÃa
Notes - Instituto de AstrofÃsica de AndalucÃa
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• Energetics of SN processes --> feedback, how much of its energy is used to reheat the<br />
gas?<br />
• In ionized regions: Photon escape? percentage?<br />
• SFR indicators and their links with time-scales<br />
• Supersonic motions and heating mechanisms in molecular clouds? kinetic temperature?<br />
• Velocity statistics and fragmentation?<br />
• (NOTE: Inclu<strong>de</strong>d after proofs... :-) ... With LMT we will be able to measure CS<br />
features at least for galactic objects. CS features, belonging to a <strong>de</strong>nser phase of the<br />
molecular gas, are crucial to <strong>de</strong>termine intensity of SF).<br />
• Can we learn something about [alpha/Fe]?<br />
• Promoting targeted surveys is a way to answer these questions. This will have to be<br />
inclu<strong>de</strong>d into methods.<br />
18:00 Discussion on the number of no<strong>de</strong>s.<br />
Things to take into account:<br />
- Money for secondments,<br />
- Money for network meetings<br />
- Money for summer schools, courses, etc.<br />
For that it would be better to have a large number of no<strong>de</strong>s.<br />
A suggestion to have no<strong>de</strong>s per topic was dropped, they are to be <strong>de</strong>fined roughly by<br />
location.<br />
The distribution in the end will probably be:<br />
o France: 3<br />
o UK: 3 (+1?) (+ associated colaborators from: Greece + The Netherlands)<br />
o Germany: 2 (+ associated from Austria?)<br />
o Spain: 3<br />
o Italy: 2<br />
o Switzerland: 1
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