Chemistry and line emission of outer protoplanetary disks

Details Chemistry and line emission of outer protoplanetary disks Chemistry and line emission of outer protoplanetary disks

2005-09-21

arxiv.org/abs/astro-ph/0509643v1

Astronomy and Astrophysics

Astrophysics

10 pages, 6 figures, to be published in the conferences proceedings of the IAU Symposium 231 on Astrochemistry

Scientific paper

The structure and chemistry of protoplanetary disks depends strongly on the nature of the central star around which it has formed. The dust temperature is mainly set by the stellar luminosity, while the chemistry of the upper disk layers depends on the amount of intercepted UV and X-ray flux. We will study the differences in chemistry, thermal sturcture and line emission around Herbig Ae/Be, T Tauri stars and low mass M dwarfs. Predictions will be made for future observations with SOFIA and Herschel.

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