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Proposal ID 011283
Title STRONG GRAVITY AND COMPLEX FE-LINE EMISSION IN SEYFERT I NUCLEI
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DOI https://doi.org/10.5270/esa-asdb4vl
Principal Investigator, PI Prof RICHARD GRIFFITHS
Abstract GT - We propose to constrain the possible contributors to the complexFe-K line emission in Sy I nuclei, where these contributors include relativistically broadened disk line emission and narrow line emission originating in a torus or other dense material in the vicinity of the nucleus.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-12-22T02:53:42Z/2001-12-02T04:28:47Z
Version 17.56_20190403_1200
Mission Description The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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 2003-01-09T00:00:00Z
Keywords "complex fe", "line emission", "narrow line emission", "dense material"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Prof RICHARD GRIFFITHS, 2003, 'STRONG GRAVITY AND COMPLEX FE-LINE EMISSION IN SEYFERT I NUCLEI', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-asdb4vl