S106: morphology and excitation of PAH, H2 and H from ISO, C10μ and BEAR

Details S106: morphology and excitation of PAH, H2 and H from ISO, C10μ and BEAR S106: morphology and excitation of PAH, H2 and H from ISO, C10μ and BEAR

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999esasp.427..707m&link_type=abstract

The Universe as Seen by ISO. Eds. P. Cox & M. F. Kessler. ESA-SP 427., p. 707

Computer Science

4

Massive Yso, S106, Pah, Molecular Gas, Imaging Fts

Scientific paper

A set of new data has been obtained on S106 with ISOCAM in CVF mode in the 6 to 9 μm range, with the ground-based mid-infrared camera C10μ and in spectro-imaging in the 2 μm region with BEAR an imaging FTS, both instruments having a 10 times better spatial resolution, i.e. ~ 0.3''. The latter data have been obtained in the Brγ and H2 1-0 S(1) lines, at a spectral resolution of ~ 15 km s-1. By comparing all these data the relation of PAH and H2 can be studied. They have on large scale the same distribution but differ in the detail. BEAR maps in the H2 and H lines show a very turbulent gas. With the velocity information provided by the BEAR data a picture of the 3D distribution of gas and dust in the S106 outflows can be built.

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