Results 111 to 120 of about 18,849 (212)

Limits on MACHOs from microlensing in the double quasar Q0957+561

open access: yes, 1998
10 pages, 4 figures, accepted by Astronomy & ...
Schmidt, Robert, Wambsganss, Joachim
openaire   +2 more sources

VODKA-JWST: Synchronized Growth of Two Supermassive Black Holes in a Massive Gas Disk? A 3.8 kpc Separation Dual Quasar at Cosmic Noon with the NIRSpec Integral Field Unit

open access: yesThe Astrophysical Journal
The search for dual supermassive black holes (SMBHs) is of immense interest in modern astrophysics. Galaxy mergers may fuel and produce SMBH pairs. Actively accreting SMBH pairs are observed as dual quasars, which are vital probes of SMBH growth.
Yuzo Ishikawa   +12 more
doaj   +1 more source

The time-delay of the gravitationally lensed double quasar UM 673

open access: yes, 2008
This paper has been ...
Akhunov, T. A.   +13 more
openaire   +2 more sources

Radio Counterparts of Ultraluminous X-Ray Sources in Nearby Galaxies

open access: yesThe Astrophysical Journal
Radio surveys of ultraluminous X-ray sources (ULXs) allow us to find supercritically accreting compact objects (SS 433/W50-like systems) or stripped nuclear black holes in nearby galaxies. We identified 21 such objects by crossmatching a ULX catalog with
Yijia Zhang   +3 more
doaj   +1 more source

A Massive Protocluster Anchored by a Luminous Quasar at z = 6.63

open access: yesThe Astrophysical Journal Letters
Protoclusters, the progenitors of galaxy clusters, trace large scale structures in the early Universe and are important to our understanding of structure formation and galaxy evolution. To date, only a handful of protoclusters have been identified in the
Feige Wang   +15 more
doaj   +1 more source

H-AMR FORGE’d in FIRE. I. Magnetic State Transitions, Jet Launching, and Radiative Emission in Super-Eddington, Highly Magnetized Quasar Disks Formed from Cosmological Initial Conditions

open access: yesThe Astrophysical Journal
Quasars are powered by supermassive black hole (SMBH) accretion disks, yet standard thin disk models are inconsistent with many observations. Recently, P. F. Hopkins et al.
Nicholas Kaaz   +4 more
doaj   +1 more source

Evidence for quasar fast outflows being accelerated at the scale of tens of parsecs. [PDF]

open access: yesSci Adv, 2022
He Z   +16 more
europepmc   +1 more source

Quasar 3C 47: Extreme Population B jetted source with double-peaked profiles

open access: yesAstronomy & Astrophysics
Context.An optically thick, geometrically thin accretion disk (AD) around a supermassive black hole might contribute to broad-line emission in type 1 active galactic nuclei (AGN). However, the emission line profiles are most often not immediately consistent with the profiles expected from a rotating disk. The extent to which an AD in AGN contributes to
Shimeles Terefe Mengistue   +5 more
openaire   +3 more sources

QuasAr Odyssey: the origin of fluorescence and its voltage sensitivity in microbial rhodopsins. [PDF]

open access: yesNat Commun, 2022
Silapetere A   +16 more
europepmc   +1 more source

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