A dataset provided by the European Space Agency

Proposal ID 010946
Title The mass of the white dwarf and physics of the accretion flows in CVs
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DOI https://doi.org/10.5270/esa-mzgmbki
Principal Investigator, PI Prof Keith Mason
Abstract GT- This is a survey of magnetic CVs, the goal of which is to determine theiroverall energy balance and, based on the temperature of the X-ray spectrum, themass of the accreting white dwarf for a large sample of objects.
Publications
Instrument RGS1, EPN, RGS2, EMOS1, OM, EMOS2
Temporal Coverage 2001-08-26T11:32:07Z/2004-09-06T07:59:52Z
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 2008-05-25T00:00:00Z
Keywords "accretion flows", "xray spectrum", "accreting white dwarf", "white dwarf", "overall energy balance", "magnetic cvs"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Prof Keith Mason, 2008, 'The mass of the white dwarf and physics of the accretion flows in CVs', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-mzgmbki