Probing Atomic and Molecular Gas in Proto-planetary Disks

Details Probing Atomic and Molecular Gas in Proto-planetary Disks Probing Atomic and Molecular Gas in Proto-planetary Disks

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009eimw.confe..43m&link_type=abstract

"The Evolving ISM in the Milky Way and Nearby Galaxies, The Fourth Spitzer Science Center Conference, Proceedings of the confere

Physics

Accretion, Accretion Disks, Infrared: Stars, Planetary Systems: Proto-Planetary Disks, Stars: Formation: Pre-Main Sequence, X-Rays: Stars, Radiative Transfer

Scientific paper

Besides being a reservoir of accreting material onto a newly formed star, the study of circumstellar disks not only shed light on the formation mechanisms of stars, but also on the formation process of planets. We discuss the expected characteristics of line emission produced in atomic and molecular gas of X-ray irradiated disks and discuss possible observables for SOFIA and Herschel.

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