| Name | 067185 |
| Title | Characterization of hard X-ray selected binaries: a census of magnetic CVs |
| URL | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0671850201 |
| DOI | https://doi.org/10.5270/esa-226vz0x |
| Author | European Space Agency |
| Description | The INTEGRAL and SWIFT satellites detected a large number of galactic X-ray sources above 20keV,among which virgul6-7% identified as accreting white dwarf binaries. Among known systems most harbour asynchronously rotating magnetic primaries, suggesting that this formerly small subclass could be an important contributor to the galactic X-ray binary populations. However, most newly discovered sources are proposed as magnetic cataclysmic variables through optical spectra. XMM-Newton demonstrated unique potential to infer their true nature through the detection of X-ray pulses and study of broad-band spectra. We propose 6 new sources that, if all confirmed as magnetics, will increase by 35% the hard X-ray sample enabling a true census of the first volume-limited sample |
| Publication | No observations found associated with the current proposal |
| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2012-01-07T15:25:52Z/2012-04-29T15:56:29Z |
| 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 | 2013-05-15T00:00:00Z |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, 2013, Characterization Of Hard X-Ray Selected Binaries: A Census Of Magnetic Cvs, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-226vz0x |