Radio and γ-ray loud narrow-line Seyfert 1 galaxies in the spotlight
Abstract
Narrow-line Seyfert 1 (NLS1) galaxies provide us with unique insights into the drivers of AGN activity under extreme conditions. Given their low black hole (BH) masses and near-Eddington accretion rates, they represent a class of galaxies with rapidly growing supermassive BHs in the local universe. Here, we present the results from our multi-frequency radio monitoring of a sample of γ-ray loud NLS1 galaxies (γNLS1s), including systems discovered only recently, and featuring both the nearest and the most distant γNLS1s known to date. We also present high-resolution radio imaging of 1H 0323+342, which is remarkable for its spiral or ring-like host. Finally, we present new radio data of the candidate γ-emitting NLS1 galaxy RX J2314.9+2243, characterized by a very steep radio spectrum, unlike other γNLS1s.
- Publication:
-
New Frontiers in Black Hole Astrophysics
- Pub Date:
- 2017
- DOI:
- arXiv:
- arXiv:1701.09111
- Bibcode:
- 2017IAUS..324..184K
- Keywords:
-
- galaxies: active;
- galaxies: jets;
- galaxies: Seyfert;
- radio continuum: galaxies;
- Astrophysics - High Energy Astrophysical Phenomena
- E-Print:
- 4 pages, 1 figure. Accepted for publication in the Proceedings of the IAU Symposium No. 324: New Frontiers in Black Hole Astrophysics