A dataset provided by the European Space Agency

Name 009363
Title Are LINERS Powered by Advection-Dominated Accretion Flows
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093630101

DOI https://doi.org/10.5270/esa-donlv90
Author Dr Kimberly Weaver
Description We propose a 15 ks observation of the LINER galaxy NGC 1052. Our goal is to provide a clean test of the ..Advection-Dominated Accretion Flow. model of low-accretion rate accretion. This can be accomplished by measuring the profile of the Fe Kalpha line---if it is relativistically broad, the disk is ..normal. all the way in to its innermost rings; a significantly narrower line would be consistent with the predictions of the ADAF model.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-08-15T01:44:36Z/2001-08-15T06:16:24Z
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 2002-09-29T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2002-09-29T00:00:00Z, 009363, 17.56_20190403_1200. https://doi.org/10.5270/esa-donlv90