File:NEWFIRM Discovery of Warm Molecular Hydrogen in the Wind of M82 (noaoann09017a).tiff

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Galaxy-scale outflows of gas (“superwinds”) are a ubiquitous phenomenon in both starburst galaxies and those containing an active galactic nucleus but the contribution from dust and molecular gas is largely unknown.

Summary[edit]

Description
English: Galaxy-scale outflows of gas (“superwinds”) are a ubiquitous phenomenon in both starburst galaxies and those containing an active galactic nucleus but the contribution from dust and molecular gas is largely unknown. (Left) “Pure”, continuum-subtracted, H2 emission on a false-color scale. (Right) Two-color image of the H2 filaments (in red) extending more than 3 kpc above and below the plane of the galaxy (shown in blue).
Date 30 November 2009 (upload date)
Source NEWFIRM Discovery of Warm Molecular Hydrogen in the Wind of M82
Author NOIRLab
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