Accretion disks are highly unstable to magnetic instabilities driven by shear flow, where classically, the axisymmetric, weak-field magnetorotational instability (MRI) has received much attention through local WKB approximations.
Nicolas Brughmans +2 more
doaj +1 more source
A tidal disruption event from an intermediate-mass black hole revealed by comprehensive multi-wavelength observations. [PDF]
Wang J +14 more
europepmc +1 more source
Extreme properties of a compact and massive accreting black hole host in the first 500 Myr. [PDF]
Tripodi R +31 more
europepmc +1 more source
Little red dots as young supermassive black holes in dense ionized cocoons. [PDF]
Rusakov V +16 more
europepmc +1 more source
Reduced gas accretion onto galaxies due to effects of external giant radio lobes. [PDF]
Qiu Y, Cen R.
europepmc +1 more source
Possible nonstellar explanation for the unexpected brightness of the earliest galaxies observed by the James Webb Space Telescope. [PDF]
Jacak JE.
europepmc +1 more source
A dormant overmassive black hole in the early Universe. [PDF]
Juodžbalis I +27 more
europepmc +1 more source
Discs no more: the morphology of low-mass simulated galaxies in FIREbox. [PDF]
Benavides JA +11 more
europepmc +1 more source
An X-ray-emitting protocluster at z ≈ 5.7 reveals rapid structure growth. [PDF]
Bogdán Á +3 more
europepmc +1 more source
Core-envelope miscibility in sub-Neptunes and super-Earths. [PDF]
Gilmore T, Stixrude L.
europepmc +1 more source

