Abstract
Using non-LTE model calculations we compute the ionization structure and hydrogen line intensity in partially ionized winds from cold (Te=4500 K) PMS stars.
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© 1988 Kluwer Academic Publishers
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Natta, A., Giovanardi, C., Palla, F. (1988). Winds from Cold Pre-Main Sequence Stars: Ionization Structure and Line Intensity. 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_38
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DOI: https://doi.org/10.1007/978-94-009-2941-8_38
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-7824-5
Online ISBN: 978-94-009-2941-8
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