Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007cxo..prop.2311c&link_type=abstract
Chandra Proposal ID #09200909
Astronomy and Astrophysics
Astronomy
Chandra Proposal Id #09200909
Scientific paper
The origin of planets is intricately tied to the evolution of primeval disks. The finer details of how the disk material evolves from an initially well-mixed distribution of gas and dust to a system composed mostly of large solids and gas giants like our own solar system is not well understood and is a fundamental question in astronomy. We can refine theories of planet formation and develop timescales for the evolution of planetary systems by studying the inner, planet-forming regions of protoplanetary disks.
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