The Fundamental Plane of GRBs - INSPIRE

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The Fundamental Plane of GRBs

Nov 15, 2023

9 pages

Published in:

Res.Astron.Astrophys. 23 (2023) 12, 125019

Published: Nov 15, 2023

DOI:

10.1088/1674-4527/ad020c

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Abstract: (IOP)

Gamma-ray bursts (GRBs) exhibit powerful radiation and relativistic jets similar to blazars. However, the central engine of GRBs remains unknown. In this paper, we use the fundamental plane to analyze a sample of GRBs with measured mass. We extend, over ∼12 orders of magnitude, the correlation analysis and fundamental plane with a sample of X-ray binaries, active galactic nuclei (AGNs) including blazars, and brightest cluster galaxies. The fundamental plane of our de-beamed sample, with a measured mass ( = (0.60 ± 0.03)+(0.78 ± 0.02)+7.23 ± 0.95), closely aligns with the findings of previous work on AGNs. This finding suggests that GRBs adhere to the fundamental plane of AGNs and supports the theory proposed in previous work that the central engine of GRBs may be black holes. This observation provides a plausible explanation for the striking similarities between GRBs and AGNs.

(stars:) gamma-ray burst: general
radiation mechanisms: general
galaxies: active

References(72)

Figures(0)

Optical and infrared polarization of active extragalactic objects

- Ann.Rev.Astron.Astrophys. 18 (1980) 321-361
•
DOI:
- 10.1146/annurev.aa.18.090180.001541

M. Arabsalmani
,
P. Møller
,
W. Freudling

- Mon.Not.Roy.Astron.Soc. 473 (2018) 3312
•
DOI:
- 10.1093/mnras/stx2451

On the mass–metallicity relation, velocity dispersion, and gravitational well depth of GRB host galaxies

et al.

- Mon.Not.Roy.Astron.Soc. 446 (2015) 990-999
•
e-Print:
- 1410.3510
•
DOI:
- 10.1093/mnras/stu2138

Constraints on a universal IMF from UV to near-IR galaxy luminosity densities

Ivan K. Baldry
(
- Johns Hopkins U.
)
,
Karl Glazebrook
(
- Johns Hopkins U.
)

- Astrophys.J. 593 (2003) 258-271
•
e-Print:
- astro-ph/0304423
•
DOI:
- 10.1086/376502

What governs the bulk velocity of the jet components in active galactic nuclei?

- Astrophys.J. 759 (2012) 114
•
e-Print:
- 1209.4702
•
DOI:
- 10.1088/0004-637X/759/2/114

Correlation between radio and broad-line emissions in radio-loud quasars

- Mon.Not.Roy.Astron.Soc. 307 (1999) 802
•
e-Print:
- astro-ph/9904322
•
DOI:
- 10.1046/j.1365-8711.1999.02657.x

A relationship between AGN jet power and radio power

et al.

- Astrophys.J. 720 (2010) 1066-1072
•
e-Print:
- 1006.5699
•
DOI:
- 10.1088/0004-637X/720/2/1066

A Radio-Selected Sample of Gamma Ray Burst Afterglows

- Astrophys.J. 746 (2012) 156
•
e-Print:
- 1110.4124
•
DOI:
- 10.1088/0004-637X/746/2/156

L. Christensen
,
P. Møller
,
J.P.U. Fynbo

- Mon.Not.Roy.Astron.Soc. 445 (2014) 225
•
DOI:
- 10.1093/mnras/stu1726

The Fundamental Plane Relation for Gamma-Ray Pulsars Implied by 4FGL

- Astrophys.J. 934 (2022) 1, 65
•
e-Print:
- 2203.13276
•
DOI:
- 10.3847/1538-4357/ac78e3

On the origin of radio emission in the x-ray states of XTE J1650-500 during the 2001-2002 outburst

Stephane Corbel
(
- Paris U., VI-VII and
- Saclay
)
,
R.P. Fender
(
- Amsterdam U., Astron. Inst.
)
,
J.A. Tomsick
(
- San Diego, CASS
)
,
Anastasios K. Tzioumis
(
- Australia, CSIRO, Epping
)
,
S. Tingay
(
- Swinburne U., Ctr. Astrophys. Supercomput.
)

- Astrophys.J. 617 (2004) 1272-1283
•
e-Print:
- astro-ph/0409154
•
DOI:
- 10.1086/425650

Coupling of the x-ray and radio emission in the black hole candidate a nd compact jet source gx 339-4

et al.

- Astron.Astrophys. 359 (2000) 251
•
e-Print:
- astro-ph/0003460

Radiatively efficient accreting black holes in the hard state: the case study of H1743-322

et al.

- Mon.Not.Roy.Astron.Soc. 414 (2011) 677
•
e-Print:
- 1101.5159
•
DOI:
- 10.1111/j.1365-2966.2011.18433.x

Integral - field spectroscopy of galactic nuclei

Tim de Zeeuw
(
- Leiden Observ.
)

- ASP Conf.Ser. 291 (2003) 205
•
e-Print:
- astro-ph/0209114

A new fundamental plane for radiatively efficient black-hole sources

- Astrophys.J.Lett. 787 (2014) L20
•
e-Print:
- 1404.5317
•
DOI:
- 10.1088/2041-8205/787/2/L20

Nucleosynthesis, Neutrino Bursts and Gamma-Rays from Coalescing Neutron Stars

David Eichler
(
- Ben Gurion U. of Negev and
- Maryland U.
)
,
Mario Livio
(
- Technion
)
,
Tsvi Piran
(
- Hebrew U. and
- Princeton U. Observ.
)
,
David N. Schramm
(
- Chicago U. and
- Fermilab
)

- Nature 340 (1989) 126-128,
•
DOI:
- 10.1038/340126a0

A Scheme to unify low - power accreting black holes: Jet - dominated accretion flows and the radio / x-ray correlation

- Astron.Astrophys. 414 (2004) 895-903
•
e-Print:
- astro-ph/0305335
•
DOI:
- 10.1051/0004-6361:20031683

A universal radio: X-ray correlation in low / hard state black hole binaries

- Mon.Not.Roy.Astron.Soc. 344 (2003) 60
•
e-Print:
- astro-ph/0305231
•
DOI:
- 10.1046/j.1365-8711.2003.06791.x

Gamma-Ray Bursts in the Swift Era

- Ann.Rev.Astron.Astrophys. 47 (2009) 567-617
•
e-Print:
- 0909.1531
•
DOI:
- 10.1146/annurev.astro.46.060407.145147

A high abundance of massive galaxies 3.6 billion years after the Big Bang

et al.

- Nature 430 (2004) 181
•
e-Print:
- astro-ph/0401037
•
DOI:
- 10.1038/nature02667

The M_(black hole)-L_(spheroid) relation at low masses

- Astrophys.J. 764 (2013) 151,
- Astrophys.J. 874 (2019) 1, 110 (erratum)
•
e-Print:
- 1211.3199
•
DOI:
- 10.1088/0004-637X/764/2/151

Low-Mass AGNs and Their Relation to the Fundamental Plane of Black Hole Accretion

- Astrophys.J.Lett. 788 (2014) 2, L22
•
e-Print:
- 1405.6986
•
DOI:
- 10.1088/2041-8205/788/2/L22

The Relationship of hard x-ray and optical line emission in low redshift active galactic nuclei

Timothy M. Heckman
(
- Johns Hopkins U.
)
,
A. Ptak
(
- Johns Hopkins U.
)
,
A. Hornschemeier
(
- Johns Hopkins U. and
- NASA, Goddard
)
,
G. Kauffmann
(
- Garching, Max Planck Inst.
)

- Astrophys.J. 634 (2005) 161-168
•
e-Print:
- astro-ph/0507674
•
DOI:
- 10.1086/491665

M.T. Hogan
,
A.C. Edge
,
J.E. Geach

- Mon.Not.Roy.Astron.Soc. 453 (2015) 1201
•
DOI:
- 10.1093/mnras/stv1517

Following the 2008 outburst decay of the black hole candidate H1743-322 in X-ray and radio

et al.

- Mon.Not.Roy.Astron.Soc. 401 (2010) 1255
•
e-Print:
- 0909.2632
•
DOI:
- 10.1111/j.1365-2966.2009.15717.x

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