GT- We aim to investigate the effect of the orientation of the magnetic field tothe incoming accretion stream on the accretion process in Polars. This willprovide information on the way the accreting material threads onto the magneticfield, and on the important physical processes taking place in the threadingregion.
Instrument
EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage
2002-03-27T17:04:14Z/2002-04-02T21:07:58Z
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.
European Space Agency, Dr Michael Watson, 2003, 'Stream-Field interactions in Magnetic CVs SSC_7', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-qxfdshf
