English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

We have explored the structure of hot magnetized accretion flow with thermalconduction. The importance of thermal conduction in hot accretion flows hasbeen confirmed by observations of the hot gas surrounding Sgr $A^*$ and a fewother nearby galactic nuclei. For a steady state structure of such accretionflows a set of self similar solutions are presented. In this paper, we haveactually tried to re-check the solution presented by Abbassi et al. (2008)using a physical constrain. In this study we find that Eq 29 places a newconstrain that limits answers presented by Abbassi et al. 2008. In that paperthe parameter space in which it is established in the new constrain wasplotted. However, the new requirement makes up only a small parameter spacewith physically acceptable solutions. And now in this manuscript we havefollowed the idea with more effort, and tried to find out how thermalconduction influences the structur of the disks in a physical parameter space.We have found out that the existence of thermal conduction will lead toreduction of accretion and radial and azimuthal velocities as well as thevertical thickness of the disk, which is slightly reduced. Moreover, thesurface density of the disk will increase when the thermal conduction becomesimportant in the hot magnetized flow.

Self-similar structure of a hot magnetized flow with thermal conduction