High resolution spectroscopy of nearby AGN
| dc.creator | Kaastra, J. S. | |
| dc.date | 2002-06-14 | |
| dc.date.accessioned | 2026-07-07T02:03:57Z | |
| dc.date.available | 2026-07-07T02:03:57Z | |
| dc.description | In this paper the potential of high resolution spectroscopy of nearby AGN with XEUS is discussed. The focus is upon the energy resolution that is needed in order to disentangle the different spectral components. It is shown that there is an urgent need for high spectral resolution, and that a spectral resolution of 1 eV, if possible, leads to a significant increase in diagnostic power as compared to 2 eV resolution. | |
| dc.description | 7 pages, 11 figures, to appear in: Proceedings of the Workshop: "XEUS - studying the evolution of the hot universe", held in Garching, March 11-13, 2002, eds. G. Hasinger, Th. Boller and A. Parmar, MPE Report | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0206237 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0206237 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/4572 | |
| dc.subject | Astrophysics | |
| dc.title | High resolution spectroscopy of nearby AGN | |
| dc.type | text |