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.
@article{arxiv.1908.00689,
title = {An Episodic Wide-angle Outflow in HH 46/47},
author = {Yichen Zhang and Hector G. Arce and Diego Mardones and Sylvie Cabrit and Michael M. Dunham and Guido Garay and Alberto Noriega-Crespo and Stella S. R. Offner and Alejandro C. Raga and Stuartt A. Corder},
journal= {arXiv preprint arXiv:1908.00689},
year = {2019}
}