Results 91 to 100 of about 719 (181)
Discovery of radio-loud quasars with z=4.72 and z=4.01 [PDF]
, 1998 I. Hook, R. G. McMahon
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Monster Radio Jet (>66 kpc) Observed in Quasar at z ∼ 5
The Astrophysical Journal LettersWe present the discovery of a large extended radio jet associated with the extremely radio-loud quasar J1601+3102 at z ∼ 5 from subarcsecond resolution imaging at 144 MHz with the International LOFAR Telescope.
Anniek J. Gloudemans +8 more
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A LARGE AREA SEARCH FOR RADIO-LOUD QUASARS WITHIN THE EPOCH OF REIONIZATION [PDF]
, 2004 M. J. Jarvis +5 more
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The Astrophysical JournalBased on the magnetization, an accretion disk with a large-scale magnetic field can be separated into either standard and normal evolution or magnetically arrested disk (MAD), which are difficult to identify from observations. It is still unclear whether
Shuang-Liang Li, Wenwen Zuo, Xinwu Cao
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Soft gamma rays from low accreting supermassive black holes and connection to energetic neutrinos. [PDF]
Nat Commun, 2021 Kimura SS, Murase K, Mészáros P.
europepmc +1 more source
High-Redshift, Radio-Loud Quasars
, 2000 I discuss two programs to study radio-loud quasars at high (z>4) redshift. Quasars are the most luminous, non-transient objects known and are observed to the earliest cosmic epochs. At lower redshifts, radio-loud quasars are associated with host galaxies having deVaucoleurs profiles. By association, identifying and studying a sample of high-redshift,
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Discovery of Radio-Loud Broad Absorption Line Quasars Using Ultraviolet Excess and Deep Radio Selection [PDF]
, 1998 M. S. Brotherton +7 more
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THE EXTREME ULTRAVIOLET DEFICIT AND MAGNETICALLY ARRESTED ACCRETION IN RADIO-LOUD QUASARS [PDF]
, 2014 Brian Punsly
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Circumgalactic Environments Around Distant Quasars 3C 9 and 4C 05.84
The Astrophysical JournalWe present results from the Quasar hosts Unveiled by high Angular Resolution Techniques survey studying the circumgalactic medium (CGM) by observing rest-frame UV emission lines Ly α , C iv , and He ii around two radio-loud quasars, 3C 9 ( z = 2.02) and ...
Sanchit Sabhlok +8 more
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Electromagnetic counterparts to massive black-hole mergers. [PDF]
Living Rev Relativ, 2022 Bogdanović T, Miller MC, Blecha L.
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