| Time |
Speaker |
Title |
| Chairman |
George Helou
|
High-z: the gas evolution |
| 8:45-9:10 |
Prochaska J. Xavier |
On the (Non)Evolution of HI Disks over Cosmic Time |
| 9:10-9:35 |
Wolfe Art |
The Schmidt Law at High Redshifts |
| 9:35-9:55 |
Rafelski Marc |
Search for Spatially Extended Star Formation around Lyman Break Galaxies in the Hubble Ultra Deep Field |
| 9:55-10:20 |
Keres Dusan |
What Drives the Cosmic Star Formation History? |
| 10:20-10:35 |
Birnboim Yuval |
Getting the gas to where we need it the most: cold streams, and their interaction with spiral galaxies |
| 10:35-10:55 |
Jorgenson Regina |
Understanding Physics Conditions in Damped Lyman alpha Systems through CI absorption lines |
| 10.55-11.25 |
|
Coffee Break in Voliera |
| 11:25-11:50 |
Blitz Leo |
The Gas Consumption History of the Universe to z = 5 |
| 11:50-12:05 |
Choi Jun-Hwan |
Cosmic star formation rate in LCDM cosmological simulation |
| 12:05-12:30 |
Kravtsov Andrey |
Modeling star formation in cosmological simulations of galaxy formation |
| 12:30-12:55 |
Schaye Joop |
Star formation laws and their role in models of the formation and evolution of
galaxies |
| 13:00-14:00 |
|
Lunch |
| Chairman |
Eve Ostriker |
Theory on SFR: from the large scale to subgrid physics |
| 14:45-15:00 |
Wong Tony |
On the Timescale for Star Formation in Galaxies |
| 15:00-15:25 |
Mac Low Mordecai-Mark |
Can't Stop the Music! Does Star Formation Only Quench When Gas is Exhausted?
|
| 15:25-15:50 |
Kim Woong-Tae |
Giant Cloud Formation and Turbulence Generation by Galactic Spiral Shocks |
| 15:50-16:05 |
Bonnell Ian |
Spiral shock triggering of star formation |
| 16:05-16:35 |
|
Icecream Break in Cortile |
| 16:35-17:00 |
Klessen Ralf |
ISM Dynamics and Star Formation |
| 17:00-17:25 |
Basu Shantanu |
Molecular Cloud Fragmentation regulated by Self-Gravity, Magnetic Fields, Ambipolar Diffusion, and Nonlinear Flows |
| 17:25-17:50 |
Vazquez-Semadeni Enrique |
Revising Key Star Formation Concepts |
| 19:30-22:30 |
|
Cena nel Casale La Sorgente |