Modern view of the warm ionized medium

Published 2 Nov 2012 in astro-ph.GA | (1211.0369v1)

Abstract: We review the observational evidence that the warm ionized medium (WIM) is a major and physically distinct component of the Galactic interstellar medium. Although up to ~20% of the faint, high-latitude H-alpha emission in the Milky Way may be scattered light emitted in midplane H II regions, recent scattered light models do not effectively challenge the well-established properties of the WIM.

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