Probing magnetohydrodynamical scenarios for jet production

Details Probing magnetohydrodynamical scenarios for jet production Probing magnetohydrodynamical scenarios for jet production

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006an....327..454d&link_type=abstract

Astronomische Nachrichten, Vol.327, Issue 5/6, p.454

Astronomy and Astrophysics

Astronomy

3

Jet-Accretion Phenomena, Magnetic Fields Origin

Scientific paper

Large-scale magnetic fields created by dynamo action along with magneto-centrifugal and reconnection processes in accretion disks around the sources is currently the most accepted mechanism for jet production. Understanding the production of magnetic fields in jet-accretion phenomena may be the key for understanding the origin of the large-scale magnetic fields in galaxy clusters and in the Universe. Here, we discuss recent observational, theoretical and numerical results on jet phenomena that support the MHD scenarios for jet production.

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