| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10696859 | Advances in Space Research | 2005 | 10 Pages |
Abstract
The presence of so many well-known interstellar molecules in solar-type hot corinos strengthens the link between molecular cloud chemistry, the starting materials of protoplanetary disks such as the protosolar nebula, and the composition of comets. Establishing the fine details of this connection is crucial in answering fundamental questions concerning the importance of galactic astrochemistry for astrobiology.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Hui-Chun Huang, Yi-Jehng Kuan, Steven B. Charnley, Naomi Hirano, Shigehisa Takakuwa, Tyler L. Bourke,