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Analytical modelling of AGN outflows

Published online by Cambridge University Press:  01 December 2004

Z. Meliani  and
C. Sauty
Z. Meliani
Affiliation:
Observatoire de Paris, L.U.Th., F-92190 Meudon, France email: zakaria.meliani@obspm.fr, christophe.sauty@obspm.fr Université de Paris 7, APC, 2 place Jussieu, F-75005 Paris, France
C. Sauty
Affiliation:
Observatoire de Paris, L.U.Th., F-92190 Meudon, France email: zakaria.meliani@obspm.fr, christophe.sauty@obspm.fr Université de Paris 7, APC, 2 place Jussieu, F-75005 Paris, France
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Abstract

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We study AGN jet formation by means of exact solutions of the relativistic magnetohydrodynamic equations. This is an original extension in Schwarzchild's metric of previous meridionally self-similar models. The outflow is mainly thermally driven to high asymptotic speeds from the central region where the escape speed is also high. The jet solutions are magnetically collimated on the sub-parsec scale.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
POSTERS
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS222 , March 2004 , pp. 459 - 460
Copyright
© 2004 International Astronomical Union