Results 101 to 110 of about 771 (176)
Radio Follow-up Observations of a Weak-line Quasar Exhibiting Remarkable X-Ray Variability
SDSS J1539+3954 ( z ≈ 1.935), a radio-quiet weak-line quasar (WLQ), exhibited exceptional X-ray variability in 2019–2020, with its X-ray flux increasing by over 20 times from 2013 to 2019 and subsequently dropping by at least a factor of 9 in 2020 ...
Ayushi Chhipa +8 more
doaj +1 more source
Based 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
doaj +1 more source
[O II] Emission, Eigenvector 1, and Orientation in Radio-quiet Quasars
We present supportive evidence that the Boroson & Green eigenvector 1 is not driven by source orientation and further that both [O III] λ5007 and [O II] λ3727 are isotropically emitted in the radio-quiet sample of bright quasar survey (BQS) quasars ...
Wilkes, Belinda +3 more
core +1 more source
The X-ray properties of the most luminous quasars with strong emission-line outflows
Context. Strong outflows from active galactic nuclei are frequently observed in objects with lower coronal X-ray luminosity. This intrinsic X-ray weakness is considered a requirement for the formation of radiatively driven winds. Aims.
Shlentsova Anastasia +9 more
doaj +1 more source
Red quasars, often associated with potent [O iii ] outflows on both galactic and circumgalactic scales, may play a pivotal role in galactic evolution and black hole feedback. In this work, we explore the [Fe ii ] emission in one such quasar at z = 0.4352–
Swetha Sankar +14 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
Windy or Not: Radio Parsec-scale Evidence for a Broad-line Region Wind in Radio-quiet Quasars
Does a broad-line region (BLR) wind in radio-quiet (RQ) active galactic nuclei (AGN) extend to parsec scales and produce radio emission? We explore the correlations between a parsec-scale radio wind and the BLR wind in a sample of 19 RQ Palomar–Green ...
Sina Chen +8 more
doaj +1 more source
UEG Week 2025 Oral Presentations
United European Gastroenterology Journal, Volume 13, Issue S8, Page S7-S188, October 2025.
wiley +1 more source
Double Lobed Radio Quasars from the Sloan Digital Sky Survey [PDF]
We have combined a sample of 44 984 quasars, selected from the Sloan Digital Sky Survey (SDSS) Data Release 3, with the FIRST radio survey. Using a novel technique where the optical quasar position is matched to the complete radio environment within 450''
de Vries, W. H. +5 more
core +1 more source
Narrow-line Seyfert 1 galaxies (NLS1s) are generally known to be radio-quiet active galactic nuclei, but a tiny subset of them are found to be extremely radio-loud with radio loudness parameter ( R _1.4 GHz ) > 100.
Veeresh Singh +3 more
doaj +1 more source

