Results 81 to 90 of about 352 (180)
FORGE'd in FIRE III: The IMF in Quasar Accretion Disks from STARFORGE
Recently, we demonstrated self-consistent formation of strongly-magnetized quasar accretion disks (QADs) from cosmological radiation-magnetohydrodynamic-thermochemical galaxy-star formation simulations, including the full STARFORGE physics shown ...
Philip F. Hopkins +5 more
doaj +1 more source
Probing the History of the Galaxy Assembly of the Counterrotating Disk Galaxy PGC 66551
Stellar counterrotation in disk galaxies directly relates to the complex phenomenon of the disk mass assembly believed to be driven by external processes, such as accretion and mergers.
Ivan Yu. Katkov +6 more
doaj +1 more source
A Sandwich Model for Changing-look Active Galactic Nuclei
The spectral variability of changing-look active galactic nuclei (CL-AGNs) occurred on timescales of years to tens of years, posing a significant challenge to the standard thin disk model. In this work, we propose a sandwich model, including an optically
Qian-Qi Ma +6 more
doaj +1 more source
The Lifetimes of High-redshift Quasars Suggest Magnetic Disk Support
It has recently been suggested that a variety of data on active galactic nuclei (AGN) can be explained if AGN disks are supported against gravitational fragmentation by magnetic fields that are advected into the disk from the surrounding galaxy.
Jarrett Johnson +4 more
doaj +1 more source
Directly Tracking the Rebrightening of a Supermassive Black Hole Accretion Disk
Accretion onto supermassive black holes (SMBHs) powers the most luminous persistent sources in the Universe, the so-called active galactic nuclei, whose emission is characterized by two distinct spectral components: thermal optical/ultraviolet (UV ...
Riccardo Middei +14 more
doaj +1 more source
The Santa Barbara Binary−disk Code Comparison
We have performed numerical calculations of a binary interacting with a gas disk, using 11 different numerical methods and a standard binary−disk setup.
Paul C. Duffell +15 more
doaj +1 more source
The Persistent Missing Mass Problem in Planet Formation
Recent ground-based microlensing surveys suggest that our Galaxy may abound with small free-floating planets, potentially up to ∼21 such planets per star. We explore the implication of such possibility on the mass budget for planet formation.
Eve J. Lee +3 more
doaj +1 more source
Electromagnetic counterparts to massive black-hole mergers. [PDF]
Bogdanović T, Miller MC, Blecha L.
europepmc +1 more source
We revisit the spectral appearance of extended self-gravitating accretion disks surrounding compact central objects such as supermassive black holes. Using dust-poor opacities, we show that all optically thick disk solutions possess a universal outer ...
Yi-Xian Chen +8 more
doaj +1 more source
H i Observations of Giant Low Surface Brightness Galaxies
Giant low surface brightness (gLSB) galaxies are galaxies with extremely extended, faint, optical disks over 50 kpc in radius and have high total masses, which can reach 10 ^12 M _⊙ .
Philip Lah +7 more
doaj +1 more source

