Physics
Scientific paper
Oct 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986inpr.conf..127s&link_type=abstract
In NASA. Ames Research Center Summer School on Interstellar Processes: Abstracts of Contributed Papers p 127-128 (SEE N87-15043
Physics
Absorptivity, Late Stars, Molecular Clouds, Protostars, Spectral Resolution, Spectrum Analysis, Ice, Particle Size Distribution, Scattering, Spectrometers, Telescopes
Scientific paper
The 3 micron absorption spectra of sources seen in or behind molecular clouds generally show a variety of absorption features. Three separate absorptions are used to explain these features. The cooled-grating array spectrometer (CGAS) at the NASA Infrared Telescope Facility was used to obtain spectra of the late-type mass-loss star OH 0739-12 and the protostars MonR2 IRS-2 and IRS-3 (solid circles). The differences between the spectra are discussed.
Sellgren Kris
Smith Gary R.
Tokunaga Alan T.
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