Gamma-ray emitting narrow-line Seyfert 1 galaxies. New discoveries and open questions
arXiv:1312.5049 · doi:10.1017/S1743921314003561
Abstract
The discovery of gamma-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-gamma-rays properties of the gamma-ray emitting narrow-line Seyfert 1 galaxies, also in comparison with the blazar scenario.
4 pages, proceedings of the IAU Symposium 304 "Multiwavelength AGN Surveys and Studies", Yerevan (Armenia)
References in corpus (6)
- Radio-Loudness of Active Galactic Nuclei: Observational Facts and Theoretical Implications
- A Comprehensive Study of 2 000 Narrow Line Seyfert 1 Galaxies from the Sloan Digital Sky Survey: I. The Sample
- Radio-loud Narrow-Line Type 1 Quasars
- A Population of Radio-loud Narrow Line Seyfert 1 Galaxies with Blazar-like Properties?
- The effect of radiation pressure on virial black hole mass estimates and the case of Narrow Line Seyfert 1 galaxies
- Multiwavelength observations of the gamma-ray emitting narrow-line Seyfert 1 PMN J0948+0022 in 2011