A dataset provided by the European Space Agency

Name 060398
Title Coronal Structure On The Road To Cataclysm
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0603980101

DOI 10.5270/esa-hbecy6r
Author Dr Jeremy Drake
Description The coronal morphology of K- and M-dwarfs in pre-cataclysmic and cataclysmic binaries is important for their angular momentum loss and evolutionary paths to novae and Type 1a supernovae. Yet very little data on the coronae of such rapidly rotating stars exists. A 55ks observation of the recently identified X-ray-bright close (p=0.3d) K4V+M1V partially eclipsing binary DV Piscium presents an excellent opportunity to investigate coronal morphology at rotation rates similar to those of CV and pre-CV secondaries, and test directly whether coronally-saturated stars are dominated by polar coronae. The observation requires the large effective area of XMM-Newton.
Publication An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities . Henley, David B., Shelton, Robin L., . ApJS . 202-14 . 2012 . 2012ApJS..202...14H ,
Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
The Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo . Miller, Matthew J., Bregman, Joel N., . ApJ . 829-9 . 2016 . 2016ApJ...829....9M ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2009-06-19T14:48:33Z/2009-06-20T06:18:46Z
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 2010-07-11T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-07-11T00:00:00Z, 060398, 17.56_20190403_1200. https://doi.org/10.5270/esa-hbecy6r