Do Outflows from the High-Mass Star-Forming Regions Favor MHD Two-Component Structure?

Details Do Outflows from the High-Mass Star-Forming Regions Favor MHD Two-Component Structure? Do Outflows from the High-Mass Star-Forming Regions Favor MHD Two-Component Structure?

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000asthe..93..545h&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 93, No. 9 Supp., p. 545 - 549 (2000)

Astronomy and Astrophysics

Astronomy

Scientific paper

Coexisting conical bipolar and equatorial outflows from the high-mass
protostar in Orion-KL have recently been discovered. The author
discusses the argument by Okamoto that this two-component outflow lends
support to his claim that all previous MHD wind theories are wrong in
suggesting self-collimating MHD flows.

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