Near-Infrared AO Spectroscopy of Edge-On Protoplanetary Disks with Subaru IRCS

Details Near-Infrared AO Spectroscopy of Edge-On Protoplanetary Disks with Subaru IRCS Near-Infrared AO Spectroscopy of Edge-On Protoplanetary Disks with Subaru IRCS

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005sao..conf..211t&link_type=abstract

Science with Adaptive Optics, Proceedings of the ESO Workshop Held at Garching, Germany, 16-19 September 2003. Edited by W. Bran

Physics

Optics

Scientific paper

We carried out near infrared (1.4-4.2 μm) AO imaging and spectroscopy of two edge-on protoplanetary disks; HK TauB and HV TauC located in Taurus molecular cloud. We found a deep H2O Ice absorption (τ~ 1.1, 1.3) for both disks, which might be attributed to cometary dust in the early stage. The resolved images show gradient of the H-K and K-L' color in the vertical direction to the disk, which is supposed to be due to the dust extinction in the protoplanetary disks.

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