A diatom model of dust in the Trapezium nebula

Details A diatom model of dust in the Trapezium nebula A diatom model of dust in the Trapezium nebula

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.140..205m&link_type=abstract

Astrophysics and Space Science (ISSN 0004- 640X), vol. 140, no. 1, Jan. 1988, p. 205-207.

Astronomy and Astrophysics

Astrophysics

1

Diatomic Molecules, Infrared Spectra, Interstellar Matter, Microorganisms, Nebulae, Grain Size, Silicon Oxides, Temperature Distribution

Scientific paper

Measurements are reported of the 5 - 35 μm infrared spectrum of a mixed diatom culture dispersed in a Cs I disc. These data are used to compute the flux from a diatom model of dust in the Trapezium nebula, where dust grain temperatures are assumed to be distributed in the range 230 - 130K. Good agreement with the observational data is found for the model.

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