8-13 micron spectrophotometry of S 106

Details 8-13 micron spectrophotometry of S 106 8-13 micron spectrophotometry of S 106

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....88..145h&link_type=abstract

Astronomy and Astrophysics, vol. 88, no. 1-2, Aug. 1980, p. 145-148.

Astronomy and Astrophysics

Astrophysics

9

Astronomical Spectroscopy, Infrared Spectra, Interstellar Matter, Nebulae, Spectrophotometry, Cosmic Dust, Emission Spectra, H Ii Regions, Hydrogen Ions, Line Spectra, Neon, O Stars, Spectrum Analysis

Scientific paper

8-13 micron spectrophotometry with mean resolution delta lambda/lambda 0.02 of three compact infrared condensations associated with the galactic H II region S 106 are presented. Strong emission in the (Ne II) lambda 12.81 micron fine-structure line has been detected. The line seems to be emitted in a moderate excitation nebula compatible with a late O-type ZAMS star as central source. The unidentified 11.3 micron emission feature appears conspicuously in the spectra. Silicate absorption at 9.7 micron is only marginally present.

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