A dataset provided by the European Space Agency

Name 010946
Title The mass of the white dwarf and physics of the accretion flows in CVs
URL

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DOI https://doi.org/10.5270/esa-mzgmbki
Author Prof Keith Mason
Description GT- This is a survey of magnetic CVs, the goal of which is to determine their overall energy balance and, based on the temperature of the X-ray spectrum, the mass of the accreting white dwarf for a large sample of objects.
Publication No observations found associated with the current proposal
Instrument EPN, OM, RGS1, RGS2, EMOS1, EMOS2
Temporal Coverage 2001-08-26T11:32:07Z/2004-09-06T07:59:52Z
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 2008-05-25T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2008-05-25T00:00:00Z, 010946, 17.56_20190403_1200. https://doi.org/10.5270/esa-mzgmbki