Mhd Simulations of Jets From Accretion Disks View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

2003

AUTHORS

Takahiro Kudoh , Ryoji Matsumoto , Kazunari Shibata

ABSTRACT

We present the MHD simulation including accretion flows in disks, acceleration of outflows from disks, and collimation of the outflows self-consistently. Although it was considered that this kind of simulations only shows the transient phenomena of jets, we found that the outflow and accretion flow reached a quasi-steady state by performing a long-term calculation in a large calculation region. Though the final stage is not exactly the steady state, the acceleration and collimation mechanisms of the outflow were the same as those of the steady theory. The scale of the calculation is approaching to the scale that was observed by the VLBI technique, which provides the current highest resolution for YSO jets. More... »

PAGES

99-102

Book

TITLE

Jets in Young Stellar Objects

ISBN

978-94-010-3764-8
978-94-007-0999-7

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/978-94-007-0999-7_16

DOI

http://dx.doi.org/10.1007/978-94-007-0999-7_16

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1038323552


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