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Title: Disk–Jet Connection in Active Supermassive Black Holes in the Standard Accretion Disk Regime

Abstract

We study the disk–jet connection in supermassive black holes by investigating the properties of their optical and radio emissions utilizing the SDSS DR7 and the NVSS catalogs. Our sample contains 7017 radio-loud quasars with detection both at 1.4 GHz and SDSS optical spectra. Using this radio-loud quasar sample, we investigate the correlation among the jet power ($${P}_{\mathrm{jet}}$$), the bolometric disk luminosity ($${L}_{\mathrm{disk}}$$), and the black hole mass ($${M}_{\mathrm{BH}}$$) in the standard accretion disk regime. We find that the jet powers correlate with the bolometric disk luminosities as $$\mathrm{log}{P}_{\mathrm{jet}}=(0.96\pm 0.012)\mathrm{log}{L}_{\mathrm{disk}}+(0.79\pm 0.55)$$. This suggests the jet production efficiency of $${\eta }_{\mathrm{jet}}\simeq {1.1}_{-0.76}^{+2.6}\,\times {10}^{-2}$$ assuming the disk radiative efficiency of 0.1, implying low black hole spin parameters and/or low magnetic flux for radio-loud quasars. But it can be also due to the dependence of this efficiency on the geometrical thickness of the accretion flow, which is expected to be small for quasars accreting at the disk Eddington ratios $$0.01\lesssim \lambda \lesssim 0.3$$. This low jet production efficiency does not significantly increase even if we set the disk radiative efficiency to be 0.3. We also investigate the fundamental plane in our samples among $${P}_{\mathrm{jet}}$$, $${L}_{\mathrm{disk}}$$, and $${M}_{\mathrm{BH}}$$. In conclusion, we could not find a statistically significant fundamental plane for radio-loud quasars in the standard accretion regime.

Authors:
ORCiD logo [1];  [1]; ORCiD logo [2];  [3];  [4]
+ Show Author Affiliations
  1. Institute of Space and Astronautical Science JAXA, Kanagawa (Japan)
  2. Hiroshima Univ., Hiroshima (Japan)
  3. Nicolaus Copernicus Astronomical Center, Warsaw (Poland)
  4. SLAC National Accelerator Lab., Stanford Univ., Menlo Park, CA (United States)
Publication Date:
Research Org.:
SLAC National Accelerator Lab., Menlo Park, CA (United States)
Sponsoring Org.:
USDOE
OSTI Identifier:
1406497
Report Number(s):
SLAC-PUB-17169
Journal ID: ISSN 1538-4357; TRN: US1703135
Grant/Contract Number:  
AC02-76SF00515
Resource Type:
Accepted Manuscript
Journal Name:
The Astrophysical Journal (Online)
Additional Journal Information:
Journal Name: The Astrophysical Journal (Online); Journal Volume: 840; Journal Issue: 1; Journal ID: ISSN 1538-4357
Publisher:
Institute of Physics (IOP)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; accretion; accretion disks; black hole physics; galaxies: active; galaxies: jets; quasars: supermassive black holes

Citation Formats

Inoue, Yoshiyuki, Doi, Akihiro, Tanaka, Yasuyuki T., Sikora, Marek, and Madejski, Grzegorz M. Disk–Jet Connection in Active Supermassive Black Holes in the Standard Accretion Disk Regime. United States: N. p., 2017. Web. doi:10.3847/1538-4357/aa6b57.
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Inoue, Yoshiyuki, Doi, Akihiro, Tanaka, Yasuyuki T., Sikora, Marek, & Madejski, Grzegorz M. Disk–Jet Connection in Active Supermassive Black Holes in the Standard Accretion Disk Regime. United States. https://doi.org/10.3847/1538-4357/aa6b57
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Inoue, Yoshiyuki, Doi, Akihiro, Tanaka, Yasuyuki T., Sikora, Marek, and Madejski, Grzegorz M. Thu . "Disk–Jet Connection in Active Supermassive Black Holes in the Standard Accretion Disk Regime". United States. https://doi.org/10.3847/1538-4357/aa6b57. https://www.osti.gov/servlets/purl/1406497.
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@article{osti_1406497,
title = {Disk–Jet Connection in Active Supermassive Black Holes in the Standard Accretion Disk Regime},
author = {Inoue, Yoshiyuki and Doi, Akihiro and Tanaka, Yasuyuki T. and Sikora, Marek and Madejski, Grzegorz M.},
abstractNote = {We study the disk–jet connection in supermassive black holes by investigating the properties of their optical and radio emissions utilizing the SDSS DR7 and the NVSS catalogs. Our sample contains 7017 radio-loud quasars with detection both at 1.4 GHz and SDSS optical spectra. Using this radio-loud quasar sample, we investigate the correlation among the jet power (${P}_{\mathrm{jet}}$), the bolometric disk luminosity (${L}_{\mathrm{disk}}$), and the black hole mass (${M}_{\mathrm{BH}}$) in the standard accretion disk regime. We find that the jet powers correlate with the bolometric disk luminosities as $\mathrm{log}{P}_{\mathrm{jet}}=(0.96\pm 0.012)\mathrm{log}{L}_{\mathrm{disk}}+(0.79\pm 0.55)$. This suggests the jet production efficiency of ${\eta }_{\mathrm{jet}}\simeq {1.1}_{-0.76}^{+2.6}\,\times {10}^{-2}$ assuming the disk radiative efficiency of 0.1, implying low black hole spin parameters and/or low magnetic flux for radio-loud quasars. But it can be also due to the dependence of this efficiency on the geometrical thickness of the accretion flow, which is expected to be small for quasars accreting at the disk Eddington ratios $0.01\lesssim \lambda \lesssim 0.3$. This low jet production efficiency does not significantly increase even if we set the disk radiative efficiency to be 0.3. We also investigate the fundamental plane in our samples among ${P}_{\mathrm{jet}}$, ${L}_{\mathrm{disk}}$, and ${M}_{\mathrm{BH}}$. In conclusion, we could not find a statistically significant fundamental plane for radio-loud quasars in the standard accretion regime.},
doi = {10.3847/1538-4357/aa6b57},
journal = {The Astrophysical Journal (Online)},
number = 1,
volume = 840,
place = {United States},
year = {Thu May 04 00:00:00 EDT 2017},
month = {Thu May 04 00:00:00 EDT 2017}
}
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  • The Astrophysical Journal, Vol. 522, Issue 1
  • DOI: 10.1086/312207

Size Dependence of the Radio-Luminosity-Mechanical-Power Correlation in Radio Galaxies
journal, May 2013

Disclosing the Radio Loudness Distribution Dichotomy in Quasars: an Unbiased Monte Carlo Approach Applied to the Sdss-First Quasar Sample
journal, October 2012

The spin of the Supermassive Black hole in ngc 3783
journal, July 2011

The Morphology of Extragalactic Radio Sources of High and Low Luminosity
journal, April 1974

  • Fanaroff, B. L.; Riley, J. M.
  • Monthly Notices of the Royal Astronomical Society, Vol. 167, Issue 1
  • DOI: 10.1093/mnras/167.1.31P

Agn jet Kinetic Power and the Energy Budget of Radio Galaxy Lobes
journal, March 2013

HIGH-SENSITIVITY 86 GHz (3.5 mm) VLBI OBSERVATIONS OF M87: DEEP IMAGING OF THE JET BASE AT A RESOLUTION OF 10 SCHWARZSCHILD RADII
journal, January 2016

Baryon Loading Efficiency and Particle Acceleration Efficiency of Relativistic Jets: Cases for low Luminosity bl lacs
journal, August 2016

Heating the hot Atmospheres of Galaxy Groups and Clusters with Cavities: the Relationship Between jet Power and Low-Frequency Radio Emission
journal, June 2011

Structure of the Accretion flow in Broad-Line Radio Galaxies: the case of 3c 390.3
journal, July 2009

THE SUZAKU VIEW OF 3C 382
journal, June 2011

Magnetic flux Paradigm for Radio Loudness of Active Galactic Nuclei
journal, February 2013

Prime Focus Spectrograph for the Subaru telescope: massively multiplexed optical and near-infrared fiber spectrograph
journal, June 2015

  • Sugai, Hajime; Tamura, Naoyuki; Karoji, Hiroshi
  • Journal of Astronomical Telescopes, Instruments, and Systems, Vol. 1, Issue 3
  • DOI: 10.1117/1.JATIS.1.3.035001

SUZAKU OBSERVATION OF THE BRIGHTEST BROAD-LINE RADIO GALAXY 4C 50.55 (IGR J21247+5058)
journal, September 2010

Black hole spin and the Radio Loud/Quiet Dichotomy of Active Galactic Nuclei
journal, February 2010

  • Tchekhovskoy, Alexander; Narayan, Ramesh; McKinney, Jonathan C.
  • The Astrophysical Journal, Vol. 711, Issue 1
  • DOI: 10.1088/0004-637X/711/1/50

The Cosmological Evolution of Quasar Black-Hole Masses
conference, January 2012

  • Mclure, R. J.; Dunlop, J. S.
  • Proceedings of the Guillermo Haro Conference 2003, Multiwavelength AGN Surveys
  • DOI: 10.1142/9789812702432_0093

The Optical-Radio Mapping: the kinetic efficiency of Radio-Loud AGNs
text, January 2007

Black Hole Spin and the Radio Loud/Quiet Dichotomy of Active Galactic Nuclei
text, January 2009

The Sloan Digital Sky Survey Quasar Catalog V. Seventh Data Release
text, January 2010

The Suzaku view of 3C 382
text, January 2011

The evolution of active galactic nuclei and their spins
text, January 2012

The contribution of spin to jet-disk coupling in black holes
text, January 2013

The Sloan Digital Sky Survey quasar catalog: tenth data release
text, January 2013

Quasar feedback and the origin of radio emission in radio-quiet quasars
text, January 2014

The power of relativistic jets is larger than the luminosity of their accretion disks
text, January 2014

The black-hole masses of Seyfert galaxies and quasars
text, January 2000

A fundamental plane of black hole activity
text, January 2003

The distribution and cosmic evolution of massive black hole spins
text, January 2004

Spectral Energy Distributions and Multiwavelength Selection of Type 1 Quasars
text, January 2006

The 2.5 m Telescope of the Sloan Digital Sky Survey
text, January 2006

The emission line - radio correlation for radio sources using the 7C Redshift Survey
text, January 1999

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    Jet Power of Jetted Active Galactic Nuclei: Implications for Evolution and Unification
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    • Pashchenko, Ilya N.; Plavin, Alexander V.
    • Monthly Notices of the Royal Astronomical Society, Vol. 488, Issue 1
    • DOI: 10.1093/mnras/stz1677

    The Properties of Parsec-scale Blazar Jets
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    Gamma-ray emitting narrow-line Seyfert 1 galaxies: Past, present, and future
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