Abstract
Very young stars, known as ‘pre-T-Tauri stars’ or ‘young stellar objects’, tend to be surrounded by elongated outflow regions involving ‘Herbig-Haro objects’. Such ‘bipolar flows’ are reminiscent of the jet-driven extragalactic radio sources. Here I collect old and new reasonings and evidences in support of the extremely relativistic nature of such flows.
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© 1993 Springer Science+Business Media Dordrecht
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Kundt, W. (1993). The Bipolar-Flow Phenomenon. In: Errico, L., Vittone, A.A. (eds) Stellar Jets and Bipolar Outflows. Astrophysics and Space Science Library, vol 186. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-1924-5_9
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DOI: https://doi.org/10.1007/978-94-011-1924-5_9
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