arXiv · 1908.00689
An Episodic Wide-angle Outflow in HH 46/47
Abstract
During star formation, the accretion disk drives fast MHD winds which usually contain two components, a collimated jet and a radially distributed wide-angle wind. These winds entrain the surrounding ambient gas producing molecular outflows. We report recent observation of 12CO (2-1) emission of the HH 46/47 molecular outflow by the Atacama Large Millimeter/sub-millimeter Array, in which we identify multiple wide-angle outflowing shell structures in both the blue and red-shifted outflow lobes. These shells are highly coherent in position-position-velocity space, extending to >40-50 km/s in velocity and 10^4 au in space with well defined morphology and kinematics. We suggest these outflowing shells are the result of the entrainment of ambient gas by a series of outbursts from an intermittent wide-angle wind. Episodic outbursts in collimated jets are commonly observed, yet detection of a similar behavior in wide-angle winds has been elusive. Here we show clear evidence that the wide-angle component of the HH 46/47 protostellar outflows experiences similar variability seen in the collimated component.
Explore related subjects
Keep this discovery
Yichen Zhang, Hector G. Arce, Diego Mardones, Sylvie Cabrit, Michael M. Dunham, Guido Garay, Alberto Noriega-Crespo, Stella S. R. Offner, Alejandro C. Raga, Stuartt A. Corder. 2019-08-02. An Episodic Wide-angle Outflow in HH 46/47. https://doi.org/10.3847/1538-4357/ab3850
Cite the original work for its findings. Save a collection to share your selection of sources.