Abstract
The problem of calculation of the accretion shock wave structure in the case of young stars is formulated physically and mathematically. Some results of its numerical solution are presented and dependence of the shock wave structure on the parameters of the problem is demonstrated. It was found that relative intensities and profiles of lines in T Tauri stars spectra depend generally speaking on velocity and density of infall gas as well as on geometry of the accretion. It is concluded that results of the calculations can be used to solve the problem of young stars activity nature. See for details Lamzin (1998).
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References
Gomez de Castro A.I., Lamzin S.A., Shatskij N.I. (1994), Astron. Reports, 71, p. 609
Lamzin S.A. (1995), Astron. and Astrophys, 295, p. L20 Lamzin S.A. (1998), Astron. Reports, in press
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© 1999 Springer Science+Business Media Dordrecht
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Lamzin, S.A. (1999). The Structure of The Shock Wave in the Case of an Accretion onto Low Mass Young Stars. In: Lago, M.T.V.T., Blanchard, A. (eds) The Non-Sleeping Universe. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4497-1_32
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DOI: https://doi.org/10.1007/978-94-011-4497-1_32
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-5923-7
Online ISBN: 978-94-011-4497-1
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