Abstract
The properties of the pre-main-sequence T Tauri stars are described in relation to the likely properties of their predecessors. These predecessors, the “pre-T Tauri stars”, are thought to be the stars responsible for exciting Herbig-Haro objects. Pre-T Tauri stars are capable of generating “stellar jets” by which bipolar flows carry material out into the ambient medium out of which low-mass stars form. Manifestations of these bipolar flows are: strings of optical Herbig-Haro objects; radio jets; large flattened dusty structures orthogonal to the flows. We describe the observations (optical, infrared, far-infrared and radio continuum) that provide evidence for these components in order to establish a framework for other authors in this volume to attempt to explain stellar and extragalactic jets by some unified model.
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© 1987 D. Reidel Publishing Company, Dordrecht, Holland
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Cohen, M. (1987). T Tauri Stars, Pre-T Tauri Stars, and Stellar Jets. In: Kundt, W. (eds) Astrophysical Jets and Their Engines. NATO ASI Series, vol 208. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-3927-1_7
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DOI: https://doi.org/10.1007/978-94-009-3927-1_7
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