Results 111 to 120 of about 18,849 (212)
Limits on MACHOs from microlensing in the double quasar Q0957+561
10 pages, 4 figures, accepted by Astronomy & ...
Schmidt, Robert, Wambsganss, Joachim
openaire +2 more sources
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
This paper has been ...
Akhunov, T. A. +13 more
openaire +2 more sources
Radio Counterparts of Ultraluminous X-Ray Sources in Nearby Galaxies
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
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
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]
He Z +16 more
europepmc +1 more source
Quasar 3C 47: Extreme Population B jetted source with double-peaked profiles
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]
Silapetere A +16 more
europepmc +1 more source

