The 3.1 micrometer ice band in infrared reflection nebulae

Details The 3.1 micrometer ice band in infrared reflection nebulae The 3.1 micrometer ice band in infrared reflection nebulae

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986inpr.conf..131p&link_type=abstract

In its Summer School on Interstellar Processes: Abstracts of Contributed Papers p 131-132 (SEE N87-15043 06-90)

Astronomy and Astrophysics

Astronomy

Astronomical Models, Ice, Infrared Astronomy, Light Scattering, Mie Scattering, Reflection Nebulae, Dust, Luminosity, Particle Size Distribution, Scattering Cross Sections, Temperature Measurement

Scientific paper

Recent observations show that infrared reflection nebulae are common phenomena in star forming regions. Extensive observations were made of two nearby infrared reflection nebulae, Orin Molecular Cloud 2 IRS1 (OMC-2/IRS1) and Cepheus A IRS6a (Cep-A/IRS6a). Mie scattering models of ice coated grains were used to study the constraints on the properties and locations of grains that could produce a feature similar to that observed in OMC-2 and Cep-A. It was concluded that scattering by ice particles alone could not be responsible for the 3.1 micron feature observed in infrared reflection nebulae.

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