Abstract
Observations of jets from young stars and of their bow shocks from the ultraviolet to centimetre wavelengths have revealed many of the characteristic properties of these objects. Here I summarize how optical imaging and spectrocopy have contributed to our understanding of the morphology, the kinematics, and the excitational state of the gas in these objects.
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Eislöffel, J. (1996). Observational properties of jets from young stars. In: Kundt, W. (eds) Jets from Stars and Galactic Nuclei. Lecture Notes in Physics, vol 471. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0102601
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DOI: https://doi.org/10.1007/BFb0102601
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