The Future of Fe-K Line Diagnostics for Probing Strong Gravity
| dc.creator | Yaqoob, T. | |
| dc.date | 2001-08-02 | |
| dc.date.accessioned | 2026-07-07T01:59:31Z | |
| dc.date.available | 2026-07-07T01:59:31Z | |
| dc.description | We review what we have learnt with ASCA from studying the Fe-K lines in AGN and describe a program to deconvolve the narrow, non-disk components of the lines with Chandra. This is necessary to derive the correct profiles of the broad, relativistic lines obtained using data from XMM and other high-throughput instruments. Since reverberation techniques are now not looking promising, we present Constellation-X simulations showing an alternative way we might be able to measure black-hole mass and spin. | |
| dc.description | To appear in Proc. of ``New Century of X-ray Astronomy'', (Japan, March 2001), eds.H. Inoue, H. Kunieda, ASP Conf. Series, in press (4 pages). Refereed | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0108032 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0108032 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/3148 | |
| dc.subject | Astrophysics | |
| dc.title | The Future of Fe-K Line Diagnostics for Probing Strong Gravity | |
| dc.type | text |