| Name | 006594 |
| Title | Structure of the Accretion Flows in Broad-Line Radio Galaxies |
| URL | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0065940101 |
| DOI | https://doi.org/10.5270/esa-8me6vkx |
| Author | European Space Agency |
| Description | We propose to observe four of the X-ray brightest broad-line radio galaxies in order to investigate the differneces between the profiles of the Fe K lines of radio-loud and radio quiet AGNs. We will obtain spectra with very high signal-to-noise ratio with EPIC so that we can fit the line profiles with disk models and determine the range of radii in the disk where the lines originate. This constitutes a test of scenarios for the difference between radio-loud and radio-quiet AGNs since such scenrios predict different disk structures and by extension different line profiles. |
| Publication | No observations found associated with the current proposal |
| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2001-03-14T12:56:44Z/2004-05-05T18:08:36Z |
| Version | 17.56_20190403_1200 |
| Mission Description | The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earth's atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis. |
| Creator Contact | https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk |
| Date Published | 2005-06-09T00:00:00Z |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, 2005, Structure Of The Accretion Flows In Broad-Line Radio Galaxies, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-8me6vkx |