Results 81 to 90 of about 272 (130)
H1517+656: The Birth of a BL Lacertae Object?
H1517+656 is an unusual source, even for a BL Lac object. It is one of the most luminous BL Lac objects known, with extreme emission properties at radio, optical, and X-ray frequencies. Furthermore, in our WFPC2 snapshot survey we discovered a series of peculiar arcs describing a 24 radius ring surrounding the source.
O'Dowd, M. +4 more
openaire +2 more sources
Revisiting the Flaring Activity in Early 2015 of BL Lacertae Object S5 0716+714
In this work, we analyzed multiwavelength data of the BL Lac object S5 0716+714 to investigate its emission mechanisms during a flaring state observed in early 2015.
Zhihao Ouyang +9 more
doaj +1 more source
HST Observations of the Host Galaxies of BL Lacertae Objects
23 pages, including 6 postscript figures and 3 tables (embedded). Latex requires aaspp4.sty and psfig.sty (not included).
URRY C. M. +5 more
openaire +3 more sources
A study of BL Lacertae objects [PDF]
K. W. Weiler, K. J. Johnston
openaire +1 more source
A 34.5 day quasi-periodic oscillation in γ-ray emission from the blazar PKS 2247-131. [PDF]
Zhou J +7 more
europepmc +1 more source
Citation-based clustering of publications using CitNetExplorer and VOSviewer. [PDF]
van Eck NJ, Waltman L.
europepmc +1 more source
The Oscillation in Evolution of Changing-look Blazar OQ 334
We investigate the evolution of a changing-look blazar (CLB) on long timescales and expect to trace the state change of a CLB. Three morphological types, including a flat spectrum radio quasar (FSRQ) state, transition state, and BL Lacertae (BL Lac ...
S. S. Ren +3 more
doaj +1 more source
Systematic Search for Long-term Trends in Fermi-LAT Jetted Active Galactic Nuclei
Jetted active galactic nuclei (AGN) exhibit variability across a wide range of timescales. Traditionally, this variability can often be modeled well as a stochastic process.
P. Peñil +5 more
doaj +1 more source
Testing viable f(R) models with the angular-diameter distance to compact quasar cores. [PDF]
Sultana J, Melia F, Kazanas D.
europepmc +1 more source

