A dataset provided by the European Space Agency

Name 000965
Title Magnetically controlled accretion in intermediate polar binaries
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0009650101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0009650201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0009650301

DOI 10.5270/esa-2z4fbqj
Author Dr Coel Hellier
Description We propose to observe two intermediate polars - AO Psc and FO Aqr - which are typical of their class, well studied, and which are among the X-ray brightest in the class. By comparing the two stars we will begin to understand why some IPs have broad iron lines and others narrow lines; why some have simple pulse profiles and others complex profiles; why some have soft components and others not, etc. We will make simultaneous observations of the hard-X-ray emitting accretion shock, the heated accretion polecap, the absorption in the shock and the accretion flow, and the optical-UV-emitting transition region between the disc and the magnetic field. The temperatures, densities,
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Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-05-12T06:00:29Z/2001-06-10T00:37:00Z
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 2002-11-03T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2002-11-03T00:00:00Z, 000965, 17.56_20190403_1200. https://doi.org/10.5270/esa-2z4fbqj