The spatial distribution of infrared radiation from visible reflection nebulae.

Details The spatial distribution of infrared radiation from visible reflection nebulae. The spatial distribution of infrared radiation from visible reflection nebulae.

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989iaus..135p.135l&link_type=abstract

IAU Symposium No. 135: Interstellar dust: contributed papers, p. 135 - 140

Physics

1

Reflection Nebulae: Infrared Radiation, Models: Infrared Radiation

Scientific paper

The authors present here results to date of studies of IRAS data on reflection nebulae selected from the van den Bergh (1966) reflection nebula sample and the van den Bergh and Herbst (1975) reflection nebula sample. Detailed scans of flux ratio and color temperature across the nebulae were obtained in order to study the spatial distribution of infrared emission. The model predictions are in good agreement with the analysis of reflection nebulae, illuminated by stars with stellar temperature ranging from 21,000K down to 3,000K.

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