20 to 40 micron spectroscopy of the Orion Nebula

Details 20 to 40 micron spectroscopy of the Orion Nebula 20 to 40 micron spectroscopy of the Orion Nebula

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974apj...193l.139h&link_type=abstract

Astrophysical Journal, vol. 193, Nov. 1, 1974, pt. 2, p. L139-L141.

Astronomy and Astrophysics

Astronomy

16

Astronomical Models, Astronomical Spectroscopy, Cosmic Dust, Infrared Astronomy, Interstellar Matter, Nebulae, Cloud Physics, Emission Spectra, Hydrogen, Line Spectra, Submillimeter Waves

Scientific paper

Attention is given to a moderate-resolution spectra of the Orion Nebula. Observational data are presented between 20 and 40 microns. Several models are shown that attempt to account for all of the observations from 20 microns to 1 mm. A model in which the dust within the molecular cloud has a clumpy distribution is given. Data show that the individual clumps have effective grain temperatures of 100 deg K and they are optically thick for wavelengths shorter than 400 microns.-

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