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http://hdl.handle.net/20.500.12386/28544
Titolo: | Prospects for gamma-ray observations of narrow-line Seyfert 1 galaxies with the Cherenkov Telescope Array | Autori: | ROMANO, Patrizia VERCELLONE, STEFANO FOSCHINI, LUIGI TAVECCHIO, Fabrizio LANDONI, Marco Knödlseder, Jurgen |
Data pubblicazione: | 2018 | Rivista: | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | Numero: | 481 | Fascicolo: | 4 | Da pagina:: | 5046 | Abstract: | Gamma-ray-emitting narrow-line Seyfert 1 (γ-NLS1) galaxies are thought to harbour relatively low-mass black holes (10<SUP>6</SUP>-10<SUP>8</SUP> M<SUB>☉</SUB>) accreting close to the Eddington limit. They show characteristics similar to those of blazars, such as flux and spectral variability in the gamma-ray energy band and radio properties which point towards the presence of a relativistic jet. These characteristics make them an intriguing class of sources to be investigated with the Cherenkov Telescope Array (CTA), the next-generation ground-based gamma-ray observatory. We present our extensive set of simulations of all currently known γ-ray emitters identified as NLS1s (20 sources), investigating their detections and spectral properties, taking into account the effect of both the extragalactic background light in the propagation of gamma-rays and intrinsic absorption components. We find that the prospects for observations of γ-NLS1 with CTA are promising. In particular, the brightest sources of our sample, SBS 0846+513, PMN J0948+0022, and PKS 1502+036, can be detected during high/flaring states, the former two even in the case in which the emission occurs within the highly opaque central regions, which prevent gamma-rays above a few tens of GeV to escape. In this case, the low-energy threshold of CTA will play a key role. If, on the other hand, high-energy emission occurs outside the broad-line region, we can detect the sources up to several hundreds of GeV - depending on the intrinsic shape of the emitted spectrum. Therefore, CTA observations will provide valuable information on the physical conditions and emission properties of their jets. | URI: | http://hdl.handle.net/20.500.12386/28544 | URL: | https://academic.oup.com/mnras/article/481/4/5046/5094611 | ISSN: | 0035-8711 | DOI: | 10.1093/mnras/sty2484 | Bibcode ADS: | 2018MNRAS.481.5046R | Fulltext: | open |
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