Abstract
Recent observations with wide field-of-view CCDs have shown that over 20 Herbig-Haro flows extend for more than one parsec from their driving sources. We review the observed properties of these giant HH flows and discuss the physical consequences for star formation, and for the physics and chemistry of the surrounding interstellar medium.
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© 1997 Springer Science+Business Media Dordrecht
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Bally, J., Devine, D. (1997). Giant Herbig-Haro Flows. In: Reipurth, B., Bertout, C. (eds) Herbig-Haro Flows and the Birth of Low Mass Stars. International Astronomical Union / Union Astronomique Internationale, vol 182. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5608-0_3
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DOI: https://doi.org/10.1007/978-94-011-5608-0_3
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