Journal article
The relativistic jet of the γ-ray emitting narrow-line Seyfert 1 galaxy 1H 0323+342
- 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.
- Publication status:
- Published
- Peer review status:
- Peer reviewed
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(Preview, Version of record, pdf, 1.4MB, Terms of use)
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- Publisher copy:
- 10.1093/mnras/stx3161
Authors
- Publisher:
- Oxford University Press
- Journal:
- Monthly Notices of the Royal Astronomical Society More from this journal
- Volume:
- 475
- Issue:
- 1
- Pages:
- 404–423
- Publication date:
- 2017-12-01
- Acceptance date:
- 2017-12-04
- DOI:
- EISSN:
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1365-2966
- ISSN:
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0035-8711
- Keywords:
- Pubs id:
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pubs:821147
- UUID:
-
uuid:5304551a-7388-4205-9e1c-20fc008b6973
- Local pid:
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pubs:821147
- Source identifiers:
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821147
- Deposit date:
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2018-01-24
- ARK identifier:
Terms of use
- Copyright holder:
- Pereira-Santaella et al
- Copyright date:
- 2017
- Notes:
- ©2017 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society
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