Abstract
Protostellar jets from intermediate- and high-mass protostars provide an excellent opportunity to understand the mechanisms responsible for intermediate- and high-mass star formation. A crucial question is if they are scaled-up versions of their low-mass counterparts. We present a detailed study of the IRAS 20126 + 4104 molecular jet, driven by a 104 L⊙ protostar. The kinematical and physical properties of the jet have been obtained by means of NIR narrow-band imaging, high resolution and low resolution IR spectroscopy. We then compare our findings with those of other high- and low-mass protostellar jets available in the literature, proposing an evolutionary scenario from low- to high-mass jets.
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© 2009 Springer-Verlag Berlin Heidelberg
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Caratti o Garatti, A., Eislöffel, J., Froebrich, D., Nisini, B., Giannini, T. (2009). Protostellar Jets Driven by Intermediate- and High-Mass Protostars: An Evolutionary Scenario?. In: Tsinganos, K., Ray, T., Stute, M. (eds) Protostellar Jets in Context. Astrophysics and Space Science Proceedings. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-00576-3_32
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DOI: https://doi.org/10.1007/978-3-642-00576-3_32
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