Abstract
We study the optical and X-ray emission from protostellar jets, focusing, in particular, on the case of HH 154. This project consists of two different and complementary approaches: the development of hydrodynamical models of the jet/ambient interaction, and the analysis of multi-wavelength observations. Comparing the results derived from the simulations with the observations we can infer the physical mechanisms leading to the complex morphology of the X-rays source observed at the base of HH 154.
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© 2009 Springer-Verlag Berlin Heidelberg
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Bonito, R., Orlando, S., Peres, G., Favata, F., Eislöffel, J. (2009). The Complex Morphology of the X-ray and Optical Emission from HH 154: The Pulsed Jet 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_42
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DOI: https://doi.org/10.1007/978-3-642-00576-3_42
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Online ISBN: 978-3-642-00576-3
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