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Gamma-ray emitting narrow-line Seyfert 1 galaxies. New discoveries and open questions
KTH, School of Engineering Sciences (SCI), Physics, Particle and Astroparticle Physics.ORCID iD: 0000-0003-0065-2933
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2014 (English)In: Proceedings of the International Astronomical Union, ISSN 1743-9213, Vol. 9, no S304, 140-143 p.Article in journal (Refereed) Published
Abstract [en]

The discovery of γ-ray emission from 5 radio-loud narrow-line Seyfert 1 galaxies revealed the presence of a possible emerging third class of AGNs with relativistic jets, in addition to blazars and radio galaxies. The existence of relativistic jets also in this subclass of Seyfert galaxies opened an unexplored research space for our knowledge of the radio-loud AGNs. Here, we discuss the radio-to-γ-rays properties of the γ-ray emitting narrow-line Seyfert 1 galaxies, also in comparison with the blazar scenario.

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2014. Vol. 9, no S304, 140-143 p.
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URN: urn:nbn:se:kth:diva-168554DOI: 10.1017/S1743921314003561ScopusID: 2-s2.0-84904979484OAI: diva2:817156

QC 20150604

Available from: 2015-06-04 Created: 2015-06-04 Last updated: 2015-06-04Bibliographically approved

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Larsson, Josefin
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