Gas in the B44 filament is accelerating away from the Upper-Sco massive stars at ~1.8 km/s/Myr, supporting the R-type filament feedback scenario.
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Accelerated gas flow along Ophiuchus B44 filament: Breaking Position-Position-Velocity degeneracy
Gas in the B44 filament is accelerating away from the Upper-Sco massive stars at ~1.8 km/s/Myr, supporting the R-type filament feedback scenario.