Daniel Kynoch
The relativistic jet of the γ-ray emitting narrow-line Seyfert 1 galaxy 1H 0323+342
Kynoch, Daniel; Landt, Hermine; Ward, Martin J; Done, Chris; Gardner, Emma; Boisson, Catherine; Arrieta-Lobo, Maialen; Zech, Andreas; Steenbrugge, Katrien; Pereira Santaella, Miguel
Authors
Dr Hermine Landt-Wilman hermine.landt@durham.ac.uk
Academic Visitor
Professor Martin Ward martin.ward@durham.ac.uk
External Examiner (PGR)
Professor Christine Done chris.done@durham.ac.uk
Professor
Emma Gardner
Catherine Boisson
Maialen Arrieta-Lobo
Andreas Zech
Katrien Steenbrugge
Miguel Pereira Santaella
Abstract
The detection of several radio-loud narrow-line Seyfert 1 (NLS1) galaxies by the Fermi Gamma-Ray Space Telescope hints at the existence of a rare, new class of γ-ray emitting active galactic nuclei with low black hole masses. Like flat spectrum radio quasars (FSRQs), their γ-ray emission is thought to be produced via the external Compton mechanism whereby relativistic jet electrons upscatter a photon field external to the jet, e.g. from the accretion disc, broad line region (BLR), and dusty torus, to higher energies. Here we study the origin of the γ-ray emission in the lowest-redshift candidate among the currently known γ-ray emitting NLS1s, 1H 0323+342, and take a new approach. We observationally constrain the external photon field using quasi-simultaneous near-infrared, optical, and X-ray spectroscopy. Applying a one-zone leptonic jet model, we simulate the range of jet parameters for which this photon field, when Compton scattered to higher energies, can explain the γ-ray emission. We find that the site of the γ-ray emission lies well within the BLR and that the seed photons mainly originate from the accretion disc. The jet power that we determine, 1.0 × 1045 erg s−1, is approximately half the accretion disc luminosity. We show that this object is not simply a low-mass FSRQ, its jet is intrinsically less powerful than predicted by scaling a typical FSRQ jet by black hole mass and accretion rate. That γ-ray-emitting NLS1s appear to host underpowered jets may go some way to explaining why so few have been detected to date.
Citation
Kynoch, D., Landt, H., Ward, M. J., Done, C., Gardner, E., Boisson, C., Arrieta-Lobo, M., Zech, A., Steenbrugge, K., & Pereira Santaella, M. (2018). The relativistic jet of the γ-ray emitting narrow-line Seyfert 1 galaxy 1H 0323+342. Monthly Notices of the Royal Astronomical Society, 475(1), 404-423. https://doi.org/10.1093/mnras/stx3161
Journal Article Type | Article |
---|---|
Acceptance Date | Dec 4, 2017 |
Online Publication Date | Dec 8, 2017 |
Publication Date | Mar 21, 2018 |
Deposit Date | Feb 2, 2018 |
Publicly Available Date | Feb 2, 2018 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 475 |
Issue | 1 |
Pages | 404-423 |
DOI | https://doi.org/10.1093/mnras/stx3161 |
Public URL | https://durham-repository.worktribe.com/output/1340298 |
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Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2017 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
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