Results 141 to 150 of about 9,238,867 (222)

RELATIONSHIP BETWEEN THE KINETIC POWER AND BOLOMETRIC LUMINOSITY OF JETS: LIMITATION FROM BLACK HOLE X-RAY BINARIES, ACTIVE GALACTIC NUCLEI, AND GAMMA-RAY BURSTS

open access: yes, 2014
The correlation between the kinetic power P-jet and intrinsic bolometric luminosity L-jet of jets may reveal the underlying jet physics in various black hole systems.
Ma, Renyi, Xie, Fu-Guo, Hou, Shujin
core  

Strong Amplitude Modulation of Hard-band X-Ray Quasiperiodic Oscillation with Soft-band Flux in RE J1034+396

open access: yesThe Astrophysical Journal
The X-ray quasiperiodic oscillation (QPO) is a remarkable form of variability in systems of compact object accretion. RE J1034+396, harboring the most significant X-ray QPO in active galactic nuclei (AGNs), is the most noteworthy source for in-depth ...
Ruisong Xia, Hao Liu, Yongquan Xue
doaj   +1 more source

4MOST Consortium Survey 6: Active galactic nuclei

open access: yes, 2019
X-ray and mid-infrared emission are signposts of the accretion of matter onto the supermassive black holes that reside at the centres of most galaxies.
McMahon, R.   +20 more
core   +1 more source

First Observational Evidence for an Interconnected Evolution between Time Lag and QPO Frequency among AGNs

open access: yesThe Astrophysical Journal Letters
Quasiperiodic oscillations (QPOs) have been widely observed in black hole X-ray binaries (BHBs), which often exhibit significant X-ray variations. Extensive research has explored the long-term evolution of the properties of QPOs in BHBs.
Ruisong Xia, Hao Liu, Yongquan Xue
doaj   +1 more source

Extreme Variability Reveals How the Eddington Ratio Regulates Coronal Power in Active Galactic Nuclei

open access: yesThe Astrophysical Journal Letters
The bolometric luminosity ( L _bol ) of active galactic nuclei (AGNs) is a key tracer of accretion physics, but its direct determination is often hindered by limited spectral coverage and contamination of the host galaxy. Bolometric corrections ( κ _λ  = 
Arghajit Jana   +15 more
doaj   +1 more source

X-ray absorption in Active Galactic Nuclei

open access: yes, 2015
I Nuclei Galattici Attivi (AGN) sono tra le sorgenti più luminose dell’Universo e sono osservati in circa 10-20% delle galassie nell’Universo locale. Il meccanismo di generazione dell’energia di queste sorgenti è l’accrescimento di materia su un buco nero supermassivo (SMBH). Secondo il paradigma del Modello Unificato (UM) il SMBH è circondato da un
openaire   +1 more source

Relation between millimeter wavelengths emission and high-energy emission for active galactic nuclei

open access: yes, 1998
After comparing the Aux densities of a sample of active galactic nuclei detected fly energetic gamma-ray experiment telescope at 90 and 230 GHz with the gamma-ray emissions detected by Compton Gamma-nay Observatory and x-ray emission, a strong ...
Huang, LH, Jiang, DR, Cao, XW
core  

Revealing an Oscillating and Contracting Compact Corona near the Event Horizon of the Supermassive Black Hole in 1ES 1927+654

open access: yesThe Astrophysical Journal Letters
Dynamic processes in the accretion flow near black holes produce X-ray flux variability, sometimes quasiperiodic. Determining its physical origin is key to mapping the accretion geometry but remains unresolved.
Qing-Cang Shui   +9 more
doaj   +1 more source

Radio Dim/Gamma-Ray Bright Active Galactic Nuclei

open access: yes, 2018
Inside virtually every large galaxy lies a supermassive black hole, known as active galactic nuclei. An especially interesting subclass of active galactic nuclei are those that emit high energy radiation.
Bohney, Amanda
core  

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