The soft X-ray excess AGN RE J2248-511
Astrophysics
2016-11-09 v1
Abstract
We model the spectral energy distribution of the ultrasoft broad-line AGN RE J2248-511 with Comptonised accretion disc models. These are able to reproduce the steep optical and ultrasoft X-ray slopes, and the derived black hole mass is consistent with independent mass estimates. This AGN displays properties of both broad and narrow line Seyfert 1 galaxies, but we conclude that it is intrinsically a `normal' Seyfert 1 viewed at high inclination angle.
Cite
@article{arxiv.astro-ph/0403008,
title = {The soft X-ray excess AGN RE J2248-511},
author = {R. L. C. Starling and E. M. Puchnarewicz and E. Romero-Colmenero},
journal= {arXiv preprint arXiv:astro-ph/0403008},
year = {2016}
}
Comments
4 pages, 1 figure. MG10 Proceedings