B44 is an R-type filament with gas flowing away from Sco-Cen stars at an acceleration of ~1.8 km/s/Myr, confirmed by deprojected velocities from two independent tracers.
The launching of cold clouds by galaxy outflows
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HST narrow-band imaging of M82's southern wind reveals a connected network of compact filaments (typical widths ~5.3 pc) whose covering fraction and flux contribution decline with height, while line ratios indicate photoionization near the disk transitioning to increasing shock heating in the diffus
citing papers explorer
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Accelerated gas flow along Ophiuchus B44 filament: Breaking Position-Position-Velocity degeneracy
B44 is an R-type filament with gas flowing away from Sco-Cen stars at an acceleration of ~1.8 km/s/Myr, confirmed by deprojected velocities from two independent tracers.
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The Small-scale Structures in the Wind of Messier 82
HST narrow-band imaging of M82's southern wind reveals a connected network of compact filaments (typical widths ~5.3 pc) whose covering fraction and flux contribution decline with height, while line ratios indicate photoionization near the disk transitioning to increasing shock heating in the diffus