Circumstellar Disks around Young Solar-type Stars

Details Circumstellar Disks around Young Solar-type Stars Circumstellar Disks around Young Solar-type Stars

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..219..385k&link_type=abstract

Stars as suns : activity, evolution and planets, Proceedings of the 219th symposium of the International Astronomical Union held

Astronomy and Astrophysics

Astronomy

Scientific paper

The chemistry of circumstellar disks around young (~10 Myr) solar-type stars is mainly driven by the strong UV radiation field of the central star. As a starting point for a detailed UV radiation field the rocket and satellite observations of the solar chromosphere are used and scaled according to the time-dependent behaviour of stellar activity. The disk chemistry as well as dust and gas temperatures are then derived self-consistently from the model. The results can be used for the identification of the most promising gas tracers as well as for the interpretation of present and future observations.

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