The abundance and thermal history of water ice in the disk surrounding HD 142527 from the DIGIT Herschel Key Program

The abundance and thermal history of water ice in the disk surrounding HD 142527 from the DIGIT Herschel Key Program

Context. The presence or absence of ice in protoplanetary disks is of great importance to the formation of planets. By enhancing solid surface density and increasing sticking efficiency, ice catalyzes the rapid formation of planetesimals and decreases the timescale of giant planet core accretion. Ai...

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Bibliographic Details
Main Authors: Min, M., Bouwman, J., Dominik, C., Waters, L. B. F. M., Pontoppidan, K. M., Hony, S., Mulders, G. D., Henning, Th., van Dishoeck, E. F., Woitke, P., Evans II, Neal J., Team, The DIGIT
Other Authors: Univ Arizona, Lunar & Planetary Lab
Language:en
Published: EDP SCIENCES S A 2016
Subjects:
protoplanetary disks
stars: individual: HD 142527
stars: pre-main sequence
Online Access:http://hdl.handle.net/10150/622159
http://arizona.openrepository.com/arizona/handle/10150/622159

Internet

http://hdl.handle.net/10150/622159
http://arizona.openrepository.com/arizona/handle/10150/622159

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