Mapping of Ices on Sub-arcminute Scales with Ground-based and Spitzer Spectroscopy

Details Mapping of Ices on Sub-arcminute Scales with Ground-based and Spitzer Spectroscopy Mapping of Ices on Sub-arcminute Scales with Ground-based and Spitzer Spectroscopy

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..357..112p&link_type=abstract

The Spitzer Space Telescope: New Views of the Cosmos ASP Conference Series, Volume 357, proceedings of the conference held 9-12

Astronomy and Astrophysics

Astronomy

Scientific paper

We discuss the method of ``ice mapping'', in which mid-infrared spectra toward multiple infrared sources located behind or in a molecular cloud core are combined to form a spatial map of the abundances of solid state species. As an example, we present an ice map of the F core in the Ophiuchus molecular cloud obtained using a combination of data from the c2d Spitzer Legacy program, VLT-ISAAC and ISOCAM-CVF. Future ice mapping projects using background stars are discussed.

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