针对NGC 1068的Seyfert 2星系X射线发射的物理一致模型
天体物理学
2007-05-23 v1
摘要
presented. A physically consistent model is developed in order to quantitatively describe the reprocessing of the central AGN continuum source into the discrete X-ray emission observed in Seyfert 2 galaxies. All the important atomic processes are taken into account, including photoexcitation, which has been neglected in some previous models. The model fits the high resolution NGC 1068 data very well, which implies that the contribution of hot collisional gas to the X-ray spectrum of NGC 1068 is negligible.
引用
@article{arxiv.astro-ph/0106398,
title = {A physically consistent model for X-ray emission by Seyfert 2 galaxies demonstrated on NGC 1068},
author = {E. Behar and A. Kinkhabwala and M. Sako and F. Paerels and S. M. Kahn and A. C. Brinkman and J. Kaastra and R. van der Meer},
journal= {arXiv preprint arXiv:astro-ph/0106398},
year = {2007}
}
备注
Submitted for the proceedings of Mass Outflows in AGNs: New Perspectives