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Astron. Astrophys. 329, 1171-1171 (1998)

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Analytical studies of collimated winds

IV. Rotating and collimated MHD outflows

E. Trussoni 1, K. Tsinganos 2 and C. Sauty 3

1 Osservatorio Astronomico di Torino, Strada dell'Osservatorio 20, I-10025 Pino Torinese (TO), Italy
2 Department of Physics, University of Crete and Research Center of Crete, P.O. Box 2208, GR-710 03 Heraklion, Crete, Greece
3 Observatoire de Paris, DAEC, URA 173, F-92195 Meudon Cedex, France

Astron. Astrophys. 325, 1099-1114 (1997)

Owing to a mistake, Fig. 10 of this paper was confused with Fig. 9, and was not printed at all. To rectify this unfortunate error, the correct Fig. 10 with its caption is reprinted below.

[FIGURE] Fig. 10. Plot of the flow speed v (in km s-1) vs the radial distance r (in cm) along the polar axis (solid line) and the outermost streamline (dashed line) for Case I ([FORMULA], [FORMULA]: upper panel) and Case II ([FORMULA], [FORMULA]: lower panel) of applications.
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© European Southern Observatory (ESO) 1998

Online publication: December 16, 1997