A collection of radial structure models of various accretion disk solutions, i.e. the radial dependence of their geometrical, physical and thermodynamic quantities. The compilation produces a linux ...

Abstract: Standard models of accretion discs study the transport of mass on a viscous time-scale but ... We solve this problem to obtain the transport rates and the vertical structure of the disc.

Abstract: We study the vertical structure of a radiation-pressure-dominated disc with a hot corona ... This effect will help to reconcile the predictions of accretion disc models with the ...

Accretion Disk: A structure formed by diffused material in orbital motion around a central body, typically formed when one star in a binary system pulls material from its companion star.

There are two major files and you are free to use any of them: Blackhole Accretion Disk_Continuous Disk.nb: This file is newer, works with Schwarzchild blackholes, JMN-1 naked singularity and possibly ...

Measuring that region is important since knowing the black hole’s mass and its accretion disk’s structure provides data that ...

The structure and behavior of the corona directly ... long been a challenge due to the overwhelming light from the accretion disk. Using NASA’s Imaging X-ray Polarimetry Explorer (IXPE ...

First Step on the Way to a Video of the Black Hole In 2019, the Event Horizon Telescope (EHT) Collaboration made history by ...

Using advanced ultraviolet imaging, astronomers discovered that the star’s accretion disk—a swirling structure feeding gas and material to the star—is far hotter and more dynamic than ...

https://doi.org/10.1086/320810 • https://www.jstor.org/stable/10.1086/320810 ABSTRACT The mass‐losing secondaries in cataclysmic binaries are progressively ...