Abstract Contents:(1) Introduction.(2) Inferences insensitive to detailed model: Some fiducial
numbers. Processes in ultrahot thermal plasma. Cyclotron/synchrotron and inverse Compton …

Powerful extragalactic radio sources comprise two extended regions containing magnetic
field and synchrotron-emitting relativistic electrons, each linked by a jet to a central compact …

Double neutron star (DNS) systems represent extreme physical objects and the endpoint of
an exotic journey of stellar evolution and binary interactions. Large numbers of DNS systems …

We present a review of the influence of cosmic repulsion and external magnetic fields on
accretion disks rotating around rotating black holes and on jets associated with these …

The explosion of ultra-stripped stars in close binaries can lead to ejecta masses< 0.1 M⊙
and may explain some of the recent discoveries of weak and fast optical transients. In Tauris …

We study super-Eddington accretion flows onto black holes using a global three-
dimensional radiation magneto-hydrodynamical simulation. We solve the time-dependent …

A new branch of equilibrium solutions for stationary accretion disks around black holes is
found. These solutions correspond to moderately super-Eddington accretion rates. The …

While apparently supplying tremendous power to their extended radio-emitting regions, the
nuclei of most radio galaxies emit little detectable radiation. It is proposed that at the centre …

Super-Eddington Accretion Disks around Supermassive Black Holes - IOPscience This site
uses cookies. By continuing to use this site you agree to our use of cookies. To find out more …

We investigate the dynamical stability of a differentially rotating disc (or torus) of fluid of
uniform entropy and uniform specific angular momentum. Such a fluid is neutrally stable to …