Unknown
Publication Date:
2019-06-27
Description:
The effects of dust inside H2 regions were studied by means of theoretical models of dusty nebulae. Infrared observations were analyzed and clear evidence was found that the emitting dust is mostly mixed with the ionized gas. Some information about the amount, distribution, and properties of dust grains was also derived.
Keywords:
ASTROPHYSICS
Type:
ESRO H2 Regions and the Galactic Centre; p 163-171
Format:
text
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