Probing The Surface Of Protoplanetary Disks Via Emission From Ionized Neon

Details Probing The Surface Of Protoplanetary Disks Via Emission From Ionized Neon Probing The Surface Of Protoplanetary Disks Via Emission From Ionized Neon

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...211.8105p&link_type=abstract

American Astronomical Society, AAS Meeting #211, #81.05; Bulletin of the American Astronomical Society, Vol. 39, p.872

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As part of the FEPS Spitzer Legacy program, we discovered four disks around sun-like stars emitting a [NeII] line at 12.81 micron. Similar detections were later reported towards other protoplanetary disks. I will present the ensemble of these results, show that emission from ionized Ne very likely originates in the hot disk atmosphere, and discuss the implications of this finding.

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