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Dust in H2 regionsThe 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.
Document ID
19750016505
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Panagia, N. (Consiglio Nazionale delle Ricerche Frascati, Italy)
Date Acquired
August 8, 2013
Publication Date
November 1, 1974
Publication Information
Publication: ESRO H2 Regions and the Galactic Centre
Subject Category
Astrophysics
Accession Number
75N24577
Funding Number(s)
CONTRACT_GRANT: NSF GP-36426X
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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