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High-spatial-resolution observations of dust and gas in NGC 7027 and the M8 hourglass

Thesis/Dissertation ·
OSTI ID:7059267
The spatial relationships among the distribution of the ionized gas, continuum dust emission, and the unidentified 3-12 ..mu..m infrared dust feature emission yield important clues to the identification of candidate grain/molecule materials responsible for feature emission, and provide observational constraints useful in the evaluation of proposed emission mechanisms. Here the results are presented of a systematic study of the 3.28-..mu..m and 3.4-..mu..m dust emission features, two of the unidentified emission bands' frequently detected in the 2-4 ..mu..m band of a variety of astronomical sources, in two energetically and morphologically dissimilar objects: the planetary nebula NGC 7027 and the M8 Hourglass HII region. Comparison and analysis of the moderate spectral resolution (..delta..lambda/lambda approx. 1%), high spatial resolution (approx. 0.4''/pixel) infrared images of NGC 7027 in the 3.28-..mu..m dust-emission feature and the Br..cap alpha.. (4.052 ..mu..m) hydrogen recombination line clearly show that the 3.28-..mu..m emission is spatially more extended than that of the ionized gas. Most of the 3.28-..mu..m feature emission arises from a thin shell, approx. 1'' thickness, at least partially outside of the HII region. Based on a simple model for the source morphology, we conclude that the 3.28-..mu.. emitters are quite robust, because they are able to survive the extremely hard ultraviolet radiation field at the interior edge of the HII region.
Research Organization:
Rochester Univ., NY (USA)
OSTI ID:
7059267
Country of Publication:
United States
Language:
English