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Deuterated H$\mathsf{_3^+}$ in proto-planetary disks

ASTRONOMY & ASTROPHYSICS, no. 2.0 (2005): 583-593

Cited: 75|Views23

Abstract

Probing the gas and dust in proto-planetary disks is central for understanding the process of planet formation. In disks surrounding solar type protostars, the bulk of the disk mass resides in the outer midplane, which is cold (= 20 K), dense (>= 10(7) cm(-3)) and depleted of CO. Observing the disk midplane has proved, therefore, to be a ...More

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