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Mapping the Outflow from G5.89-0.39 in SiO(5-4)

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arxiv astro-ph/0403524 v1 pith:2GMICNZB submitted 2004-03-22 astro-ph

P. K. Sollins , T. R. Hunter , J. Battat , H. Beuther , P. T. P. Ho , J. Lim , S. Y. Liu , N. Ohashi
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T. K. Sridharan Y. N. Su J.-H. Zhao Q. Zhang
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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.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 33 citations worldwide. Full citation record

  1. Explosive Molecular Outflows

    astro-ph.SR 2026-07 accept novelty 4.5 of 10

    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.

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