A high spatial resolution map of the Orion Nebula at 33 microns

Details A high spatial resolution map of the Orion Nebula at 33 microns A high spatial resolution map of the Orion Nebula at 33 microns

Jan 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978a%26a....62..261b&link_type=abstract

Astronomy and Astrophysics, vol. 62, no. 1-2, Jan. 1978, p. 261-263.

Astronomy and Astrophysics

Astronomy

14

Astronomical Maps, Infrared Astronomy, Nebulae, Astronomical Models, Flux (Rate), Protostars, Radiant Flux Density, Silicates

Scientific paper

A 33 micron map of the Orion Nebula showing the Kleinmann-Low Nebula and the Trapezium region at high spatial resolution is presented. The emission from the Trapezium can be explained by radiation from a single temperature grain population with long wavelength characteristics similar to known silicates. The Kleinmann-Low Nebula appears larger at 33 microns than at 20 microns, in accordance with predictions of a model for KL as a centrally heated, optically thick cloud. An upper limit to the emission from the Becklin-Neugebauer point source is set.

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