University of New South Wales, Sydney, NSW 2052, Australia; firstname.lastname@example.org
Beneath the familiar surface of the Orion Nebula is a spectacular molecular hydrogen outflow from a young stellar object, of very unusual morphology. In this paper I briefly discuss this outflow, its possible origins, and its interaction with the Nebula.
(Received September 15 2000)
(Accepted November 24 2000)