CVF spectral photometry of the H2 region S 106

Details CVF spectral photometry of the H2 region S 106 CVF spectral photometry of the H2 region S 106

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982esasp.192...17e&link_type=abstract

In ESA Galactic and Extragalactic Infrared Spectroscopy p 17-20 (SEE N83-18593 08-88)

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Infrared Spectroscopy, Nebulae, Stellar Spectra, Stellar Spectrophotometry, Infrared Radiation, Ions, Spectrum Analysis

Scientific paper

New 2-4 and 8-13 micron spectra of the bipolar nebula S 106 are reported, as well as observations of the lambda 12.8 micron NeII line and the 11.3 micron unidentified emission feature. HI recombination lines are observed at the infrared point source and in the optical lobes. The Ne line shows a good correspondance with the radio continuum, but with some marked differencies. Very prominent in the spectrum of the lobes are the 3.3 and 3.4 micron emission features. These are the first observations of the 3.4 micron feature. Results of the 11.3 micron feature show that the feature carrier is widely present in this object. No evidence of the 9.7 micron silicate absorption is found. For the point source, the 8-13 micron spectrum can be easily explained by means of other observed physical processes.

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