Crystalline Silicates in Circumstellar Accretion Disks

Computer Science

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Scientific paper

This research program, which includes 10 hours of SIRTF observing time, is designed to study the effects of processing of ice and dust in proto-planetary systems. Spectroscopic observations with SIRTF's Infrared Spectrograph obtained from the "Cores to Disks" Legacy Science project will be combined with new SED observations from the Multiband Imaging Photometer for SIRTF to determine the major dust and ice components throughout the star formation process. The sensitivity of SIRTF will enable observations of silicates around a variety of solar-type post-main sequence stars and ices in very young stellar objects and in edge-on disks. These observations are SIRTF Fellow guaranteed time.

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