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Related papers: Interpreting the radio/X-ray correlation of black …

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Recently a correlation between the radio and X-ray luminosities is found, $L_{\rm R}\propto L_{\rm X}^{0.7}$, in black hole sources including black hole candidates in our galaxy and active galactic nuclei. We first show that the correlation…

Astrophysics · Physics 2009-11-10 Feng Yuan , Wei Cui

We present a novel method to measure the accretion rate of radio emitting X-ray binaries (XRBs) and active galactic nuclei (AGN) independently of the X-ray luminosity. The radio emission of the jet is used as a tracer for the accretion rate…

Astrophysics · Physics 2009-11-11 Elmar Koerding , Rob Fender , Simone Migliari

When the matter from a companion star is accreted towards the central compact accretor, i.e. a black hole (BH) or a neutron star (NS), an accretion disc and a jet outflow will form, providing bight X-ray and radio emission, which is known…

High Energy Astrophysical Phenomena · Physics 2023-03-21 Pei-Xin Shen , Wei-Min Gu

We examine the disc--jet connection in stellar mass and supermassive black holes by investigating the properties of their compact emission in the X-ray and radio bands. We compile a sample of ~100 active galactic nuclei with measured mass,…

Astrophysics · Physics 2011-05-05 Andrea Merloni , Sebastian Heinz , Tiziana Di Matteo

The observed tight radio/X-ray correlation in the low spectral state of some black hole X-ray binaries implies the strong coupling of the accretion and jet. The correlation of $L_{\rm R} \propto L_{\rm X}^{\sim 0.5-0.7}$ was well explained…

High Energy Astrophysical Phenomena · Physics 2015-06-23 Erlin Qiao , B. F. Liu

Optically thin and geometrically thick accretion flows are known to be responsible for the observed radio/X-ray luminosity relation of the X-ray bright galactic nuclei. It has also been suggested that supermassive black hole masses can be…

Astrophysics · Physics 2009-11-07 Heon-Young Chang , Chul-Sung Choi , Insu Yi

A tight correlation between the radio and X-ray emission in the hard state of black hole X-ray binaries (BHXRBs) indicates an intrinsic disc-jet connection in stellar black hole accretion systems, though the detailed physics processes at…

High Energy Astrophysical Phenomena · Physics 2024-08-21 Yiheng Jiang , Shanshan Li , Xinwu Cao , Bei You , Andrzej A. Zdziarski , Saien Xu

The correlation between radio and X-ray luminosity in the hard state of black hole X-ray binaries is important for unveiling the relation between the accretion flow and the jets. In this paper, we have modeled the quasi-simultaneous…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Renyi Ma

Recent studies of the cosmic X-ray background (XRB) have suggested the possible existence of a population of relatively faint sources with hard X-ray spectra; however, the emission mechanism remains unclear. If the hard X-ray emission is…

Astrophysics · Physics 2007-05-23 Insu Yi , Stephen P. Boughn

Black hole accretion and jet production are areas of intensive study in astrophysics. Recent work has found a relation between radio luminosity, X-ray luminosity, and black hole mass. With the assumption that radio and X-ray luminosity are…

High Energy Astrophysical Phenomena · Physics 2009-11-13 Kayhan Gultekin , Edward M. Cackett , Jon M. Miller , Tiziana Di Matteo , Sera Markoff , Douglas O. Richstone

Radio and X-ray fluxes of accreting black holes in their hard state are known to correlate over several orders of magnitude. This correlation however shows a large scatter: black hole candidates with very similar X-ray luminosity, spectral…

High Energy Astrophysical Phenomena · Physics 2015-05-13 Piergiorgio Casella , Asaf Pe'er

We examine the X-ray - radio correlation in Galactic black hole sources. We highlight some of the results which extend the flux-flux relations to sources with very high accretion rates. Some of the recent results indicate that the…

Astrophysics · Physics 2008-11-26 A. R. Rao

We investigate the correlation between 151 MHz radio luminosity, L_151MHz, and jet power, P_jet, for a sample of low-power radio galaxies, of which the jet power is estimated from X-ray cavities. The jet power for a sample of FR I radio…

High Energy Astrophysical Phenomena · Physics 2015-05-27 Qingwen Wu , Xinwu Cao , Ding-Xiong Wang

We explore the evolution in power of black holes of all masses, and their associated jets, within the scheme of an accretion rate-dependent state transition. Below a critical value of the accretion rate all systems are assumed to undergo a…

Astrophysics · Physics 2008-11-26 Heino Falcke , Elmar Koerding , Sera Markoff

The accretion/ejection coupling in accreting black hole binaries has been described by empirical relations between the X-ray/radio and X-ray/optical-infrared luminosities. These correlations were initially thought to be universal. However,…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Paolo Soleri , Rob Fender

The radio/X-ray correlation is one of the most important pieces of observational evidence of the disk-jet connection in accreting compact objects. However, a growing number of X-ray binaries seem to present deviations from the universal…

High Energy Astrophysical Phenomena · Physics 2019-01-30 Karri I. I. Koljonen , David M. Russell

It has been suggested that optically thin and geometrically thick accretion flows are responsible for the observed radio/X-ray luminosity relation of the X-ray bright galactic nuclei. If this is the case then central supermassive black hole…

Astrophysics · Physics 2007-05-23 Heon-Young Chang , Chul-Sung Choi , Insu Yi

Relationships between the X-ray and radio behavior of black hole X-ray binaries during outbursts have established a fundamental coupling between the accretion disks and radio jets in these systems. We begin by reviewing the prevailing…

In this paper I review the results of our ongoing project to investigate the coupling between accretion disk and radio jet in galactic nuclei and stellar mass black holes. We find a good correlation between the UV bump luminosity and the…

Astrophysics · Physics 2015-06-24 Heino Falcke

Observationally, for neutron star low-mass X-ray binaries, so far, the correlation between the radio luminosity $L_{\rm R}$ and the X-ray luminosity $L_{\rm X}$, i.e., $L_{\rm R}\propto L_{\rm X}^{\beta}$, has been reasonably…

High Energy Astrophysical Phenomena · Physics 2019-05-29 Erlin Qiao , B. F. Liu
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