Abstract
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.
Original language | English |
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Pages | 87 |
Publication status | Published - May-2011 |
Event | 280th Symposium of the International Astronomical Union - Toledo, Spain Duration: 30-May-2011 → 3-Jun-2011 |
Conference
Conference | 280th Symposium of the International Astronomical Union |
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Country/Territory | Spain |
City | Toledo |
Period | 30/05/2011 → 03/06/2011 |