X-rays impact protoplanetary disks hydrostatic, thermal and chemical structure. The range of efficiency of X-rays is explored using a grid modelling approach: different parameters affects the structure of the disk, this determines different contribution of the X-ray radiation to the chemistry and thermal equilibrium. These contribution is studied in a systematic way focusing the attention on the line emission of different tracers.
|Publication status||Published - May-2011|
|Event||280th Symposium of the International Astronomical Union - Toledo, Spain|
Duration: 30-May-2011 → 3-Jun-2011
|Conference||280th Symposium of the International Astronomical Union|
|Period||30/05/2011 → 03/06/2011|