Abstract
Jets and winds in pre-main sequence (PMS) stars are often heated and ionized, and understanding their heating mechanism is desired to compare UV-to-IR spectral signatures with models and thus investigate their driving mechanism. We review our results of long-slit spectroscopy and spectro-astrometry for He I 1.083 μm and Hα emission, and investigate the heating mechanisms in the jet in the outer (> 10 AU) and inner (< 10 AU) regions, respectively.
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Takami, M., Chrysostomou, A., Bailey, J., Gledhill, T., Tamura, M., Terada, H. (2003). Hα and Hei Emission in the Jets of Pre-Main Sequence Stars — Implications for the Heating Mechanisms. In: Fernandes, A.J.L., Garcia, P.J.V., Lima, J.J.G. (eds) Jets in Young Stellar Objects. Springer, Dordrecht. https://doi.org/10.1007/978-94-007-0999-7_23
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DOI: https://doi.org/10.1007/978-94-007-0999-7_23
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-3764-8
Online ISBN: 978-94-007-0999-7
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