Abstract
High-resolution long-slit spectra of the HH 24 complex are presented. The data reveal the presence of a bipolar system of jet-type mass flows emanating from the infrared source SSV 63 considered to be the “exciting” star of HH 24. The detailed position-velocity (PV) structure derived for the jet-like component HH 24C is compared with a kinematical model of highly collimated mass flow consisting of a cylindric inner core and a co-axial envelope. In the course of propagation along the flow axis, the core presents a nearly constant velocity, whereas significant deceleration is found in the envelope.
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© 1988 Kluwer Academic Publishers
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Solf, J. (1988). High-Resolution Spectroscopy of Jets from Young Stars. In: Bianchi, L., Gilmozzi, R. (eds) Mass Outflows from Stars and Galactic Nuclei. Astrophysics and Space Science Library, vol 142. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2941-8_43
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DOI: https://doi.org/10.1007/978-94-009-2941-8_43
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-7824-5
Online ISBN: 978-94-009-2941-8
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