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Relativistic jets in 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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2013 (English)In: EPJ Web of Conferences: The Innermost Regions of Relativistic Jets and Their Magnetic Fields, EDP Sciences, 2013, 05006- p.Conference paper (Refereed)
Abstract [en]

Before the launch of the Fermi satellite only two classes of AGNs were known to produce relativistic jets and thus emit up to the γ-ray energy range: blazars and radio galaxies, both hosted in giant elliptical galaxies. The first four years of observations by the Large Area Telescope on board Fermi confirmed that these two are the most numerous classes of identified sources in the extragalactic γ-ray sky, but 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. Considering that narrow-line Seyfert 1 galaxies seem to be typically hosted in spiral galaxy, this finding poses intriguing questions about the nature of these objects, the onset of production of relativistic jets, and the cosmological evolution of radio-loud AGN. 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.

Place, publisher, year, edition, pages
EDP Sciences, 2013. 05006- p.
, EPJ Web of Conferences, ISSN 2101-6275 ; 61
National Category
Physical Sciences
URN: urn:nbn:se:kth:diva-143150DOI: 10.1051/epjconf/20136105006ISI: 000343671600051ScopusID: 2-s2.0-84893270285OAI: diva2:706159
International Symposium on the Innermost Regions of Relativistic Jets and Their Magnetic Fields; Granada; Spain; 10 June 2013 through 14 June 2013

QC 20140319

Available from: 2014-03-19 Created: 2014-03-17 Last updated: 2015-10-06Bibliographically approved

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Larsson, Josefin
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Particle and Astroparticle Physics
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