| Precise if your presentation is oral or a poster : | Poster |
| Title of your presentation : | Impact of gas cooling on high redshift structure formation |
| Abstract |
|
Gas coooling (both molecular and atomic) is the key ingredient to properly model barionic objects and to understand their formation. Results of high resolution early structure formation (SF) simulations will be presented and the impact on SF history of different types of modeling will be discussed. |
