Hostname: page-component-cd9895bd7-p9bg8 Total loading time: 0 Render date: 2024-12-31T13:39:18.328Z Has data issue: false hasContentIssue false
  • English
  • Français

The astrophysical jets

Published online by Cambridge University Press:  24 February 2011

Wolfgang Kundt
Wolfgang Kundt*
Affiliation:
Argelander Institute of Bonn University, Auf dem Hügel 71, D-53121 Bonn, Germany email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

In this published note I attempt to sketch my understanding of the universal working scheme of all the astrophysical jet sources, or ‘bipolar flows’, on both stellar and galactic scales, also called ‘microquasars’, and ‘quasars’. A crucial building block will be their medium: extremely relativistic e±-pair plasma performing quasi loss-free E × B-drifts through self-rammed channels, whose guiding equi-partition E- and B-fields convect the electric potential necessary for eventual single-step post-acceleration, at their terminating ‘knots’, or ‘hotspots’. The indispensible pair plasma is generated in magnetospheric reconnections of the central rotator. Already for this reason, black holes cannot serve as jet engines.

Keywords

black hole physicsplasmasISM: jets and outflowsgalaxies: jets
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S275: Jets at all Scales , September 2010 , pp. 92 - 93
Copyright
Copyright © International Astronomical Union 2011

References

Blome, H.-J., Kundt, W., 1988, Astrophys. & Space Sci., 148, 343–361CrossRefGoogle Scholar
de G. Dal Pino, E. M., Piovezan, P. P., Kadowaki, L. H. S. 2010, Astron. Astrophys., 518; arXiv:1005.3067v1Google Scholar
Kaiser, C. R. & Hannikainen, D. C. 2002, MNRAS, 330, 225–231CrossRefGoogle Scholar
Körding, E. G., & Jester, S., & Fender, R. 2006, MNRAS, 372, 1366–1378CrossRefGoogle Scholar
Körding, E. G., Jester, S., & Fender, R. 2008, MNRAS, 383, 277–288Google Scholar
Komossa, S. 2005, in Growing Black Holes, ESO Symposia, Springer, 159–163Google Scholar
Kulsrud, R. M., Ostriker, J. P., & Gunn, J. E. 1972, Phys. Rev. Lett., 28, 636–639CrossRefGoogle Scholar
Kundt, W. 1979, Astrophys. & Space Science, 62, 335–345Google Scholar
Kundt, W. 1990, Astrophys. & Space Sci., 172, 109–134CrossRefGoogle Scholar
Kundt, W. 1996, in Jets from Stars and Galactic Nuclei, Lecture Notes in Physics 471, Springer, Kundt, W. (ed.), 140–144Google Scholar
Kundt, W. 2001, in MICROQUASARS, Proceedings of the Third Miroquasar Workshop, Castro-Tirado, A.J., Greiner, J. & Paredes, J.M. (eds.), Kluwer, 273–277Google Scholar
Kundt, W. 2005, Astrophysics, A New Approach, Springer, Chapter 11Google Scholar
Kundt, W. 2009a, in XIIIth Brazilian School of Cosmology & Gravitation, AIP Conf. Proc. 1132, Novello, M. & Bergliaffa, S.E.P. (eds.), Melville, N.Y., 288–302Google Scholar
Kundt, W. 2009b, in General Relativity and Gravitation, 1967-1980, 9, 41Google Scholar
Kundt, W. & Gopal-Krishna, 1980, Nature, 288, 149–150.Google Scholar
Kundt, W. & Krishna, G. 2004, J. Astrophys. Astr., 25, 115–127CrossRefGoogle Scholar