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Chemistry and Line Emission of Outer Protoplanetary Disks by Kamp, Inga; Dullemond, Cornelis P.; Hogerheijde, Michiel; Enriquez, Jesus Emilio is a scholarly article available to read on EtoBox.

What is Chemistry and Line Emission of Outer Protoplanetary Disks about?

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.

Author

Kamp, Inga; Dullemond, Cornelis P.; Hogerheijde, Michiel; Enriquez, Jesus Emilio

Published

2005

Language

EN