A dataset provided by the European Space Agency

Name 030531
Title COMMON ENVELOPE EVOLUTION AND CORONAL ERSATURATION
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305310101

DOI 10.5270/esa-jo2f8u6
Author Dr Jeremy Drake
Description We propose to obtain the first high resolution X-ray spectra of the fastest rotating stars outside of accreting systems: the secondaries of pre-cataclysmic variables that are thought to have undergone common envelope evolution. The resulting data will: (1) Provide C and N abundances with which to perform a definitive test of common envelope evolution theory for pre-cataclysmic binaries; (2) Probe the phenomenon of ''supersaturation.. and coronal morphology, temperature structure and abundances at rotation rates a factor of two greater than studied to date. This coronal activity is responsible for the angular momentum loss that ultimately leads to Roche lobe overflow and accretion.
Publication The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C., et all. . A&A . 493-339 . 2009 . 2009A&A...493..339W ,
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 2009A&A...496..879M ,
Detection of Accretion X-Rays from QS Vir: Cataclysmic or a Lot of Hot Air? . Matranga, Marco, Drake, Jeremy J., et all. . ApJ . 747-132 . 2012 . 2012ApJ...747..132M ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
Hard X-ray Emission Associated with White Dwarfs. III. . Bilikova, Jana, Chu, You-Hua, et all. . AJ . 140-1433 . 2010 . 2010AJ....140.1433B ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
Cool X-ray emitting gas in the core of the Centaurus cluster of galaxies . Sanders, J. S., Fabian, A. C., et all. . MNRAS . 385-1186 . 2008 . 2008MNRAS.385.1186S ,
The XMM Cluster Survey: X-ray analysis methodology . Lloyd-Davies, E. J., Romer, A. Kathy, et all. . MNRAS . 418-14 . 2011 . 2011MNRAS.418...14L ,
Automatic Classification of Time-variable X-Ray Sour...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2006-01-25T18:14:25Z/2006-01-27T03:25:00Z
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 2007-02-12T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2007-02-12T00:00:00Z, 030531, 17.56_20190403_1200. https://doi.org/10.5270/esa-jo2f8u6