Mid-infrared PAH and H2 emission as a probe of physical conditions in extreme PDRs
arXiv:0910.3935 · doi:10.1088/0004-637X/706/1/L160
Abstract
Mid-infrared (IR) observations of polycyclic aromatic hydrocarbons (PAHs) and molecular hydrogen emission are a potentially powerful tool to derive physical properties of dense environments irradiated by intense UV fields. We present new, spatially resolved, \emph{Spitzer} mid-IR spectroscopy of the high UV-field and dense photodissocation region (PDR) around Monoceros R2, the closest ultracompact \hII region, revealing the spatial structure of ionized gas, PAHs and H emissions. Using a PDR model and PAH emission feature fitting algorithm, we build a comprehensive picture of the physical conditions prevailing in the region. We show that the combination of the measurement of PAH ionization fraction and of the ratio between the H 0-0 S(3) and S(2) line intensities, respectively at 9.7 and 12.3 m, allows to derive the fundamental parameters driving the PDR: temperature, density and UV radiation field when they fall in the ranges K, cm, respectively. These mid-IR spectral tracers thus provide a tool to probe the similar but unresolved UV-illuminated surface of protoplanetary disks or the nuclei of starburst galaxies.
Accepted for publication in ApJ Letters
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