Probing Protoplanetary Disk Upper Atmospheres for Heating and Dust Settling using Synthetic CO Spectra

Details Probing Protoplanetary Disk Upper Atmospheres for Heating and Dust Settling using Synthetic CO Spectra Probing Protoplanetary Disk Upper Atmospheres for Heating and Dust Settling using Synthetic CO Spectra

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010jsara...4...20l&link_type=abstract

Journal of the Southeastern Association for Research in Astronomy, vol. 4, p. 20-25

Astronomy and Astrophysics

Astronomy

Circumstellar Matter, Line: Profiles, Planetary Systems: Protoplanetary Disks, Stars: Individual (Hd 100546, Hd 1415469, Hd 97048), Stars: Individual: Hd 100546, Hd 1415469, Hd 97048

Scientific paper

CO emission is a useful probe of the warm gas distribution in the planet forming regions of disks around Herbig Ae/Be (HAeBe) stars. We model UV fluoresced and thermally excited CO in the circumstellar disks of several HAeBes. We find indications of dust settling in the upper atmospheres of HD 141569 and HD 97048 and a correlation between PAH luminosity and gas heating in these two systems.

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