Influence of self-gravity on the equilibrium structures of magnetized tori

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F17%3A00484614" target="_blank" >RIV/67985815:_____/17:00484614 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1017/S174392131700148X" target="_blank" >http://dx.doi.org/10.1017/S174392131700148X</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1017/S174392131700148X" target="_blank" >10.1017/S174392131700148X</a>

Result language
angličtina
Original language name
Influence of self-gravity on the equilibrium structures of magnetized tori
Original language description
We present some results obtained with a toy model developed in Trova et al. 2016 used to study the influence of the self-gravity onnthe equilibrium configurations of magnetized rotating self-gravitating gaseous tori, in the context of gaseous/dusty tori surrounding super-nmassive black holes in galactic nuclei. While the central black hole dominates the gravitational field and it remains electrically neutral, the surrounding material has a non-negligible self- gravitational effect on the torus structure. The vertical and radial struninfluenced by the balance between the gravitational and the magnetic force. By comparison with a previous work without self-gravity (Slany et al. 2016), we show that the conditions of existenceof these configurations can change.
Czech name
—
Czech description
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Project
<a href="/en/project/GB14-37086G" target="_blank" >GB14-37086G: Albert Einstein Center for Gravitation and Astrophysics</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Publication year
2017
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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