Explosive molecular outflows are short-lived isotropic events in massive clusters, driven by protostellar disruptions or mergers, occurring roughly once every 140 years in the Galaxy.
Mapping the Outflow from G5.89-0.39 in SiO(5-4)
1 Pith paper cite this work, alongside 33 external citations. Polarity classification is still indexing.
1
Pith paper citing it
33
external citations · Pith
abstract
We have mapped the ultracompact HII region, G5.89-0.39, and its molecular surroundings with the Submillimeter Array at 2".8 x 1".8 angular resolution in 1.3 mm continuum, SiO(5-4), and eight other molecular lines. We have resolved for the first time the highly energetic molecular outflow in this region. At this resolution, the outflow is definitely bipolar and appears to originate in a 1.3 mm continuum source. The continuum source peaks in the center of the HII region. The axis of the outflow lines up with a recently discovered O5V star.
fields
astro-ph.SR 1years
2026 1verdicts
ACCEPT 1representative citing papers
citing papers explorer
-
Explosive Molecular Outflows
Explosive molecular outflows are short-lived isotropic events in massive clusters, driven by protostellar disruptions or mergers, occurring roughly once every 140 years in the Galaxy.