2.5D Nonsteady MHD Simulations of Magnetically Driven Jets from Accretion Disks by Using the CIP-MOCCT Method View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

1999

AUTHORS

T. Kudoh , K. Shibata , R. Matsumoto

ABSTRACT

Astrophysical jets have been observed in young stellar objects (YSOs), active galactic nuclei (AGNs), and some X-ray binaries (XRBs). Although the acceleration and collimation mechanisms of these jets are still not well understood, these objects are believed to have accretion disks in their central regions. One of the most promising models for jet formation is magnetic acceleration from accretion disks (Blandford & Payne, 1982; Uchida & Shibata, 1985; Shibata Sz Uchida, 1986; Stone & Norman, 1994; Meier et al., 1997). We present the results of 2.5-dimensional MHD simulations of jet formation by magnetic accretion disks in which both ejection and accretion of disk plasma are included self- consistently. More... »

PAGES

203-206

References to SciGraph publications

Book

TITLE

Numerical Astrophysics

ISBN

978-94-010-6008-0
978-94-011-4780-4

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/978-94-011-4780-4_63

DOI

http://dx.doi.org/10.1007/978-94-011-4780-4_63

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1038661077


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