Probing the Gas in the Planet Forming Regions of Protoplanetary Disks

Astronomy and Astrophysics – Astronomy

Scientific paper

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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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