A dataset provided by the European Space Agency

Name 011125
Title Stream-Field interactions in Magnetic CVs SSC_7
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111250101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111251401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111251501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111251601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111251701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111251801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111251901

DOI 10.5270/esa-qxfdshf
Author Dr Michael Watson
Description GT- We aim to investigate the effect of the orientation of the magnetic field to the incoming accretion stream on the accretion process in Polars. This will provide information on the way the accreting material threads onto the magnetic field, and on the important physical processes taking place in the threading region.
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 ,
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 ,
The energy balance of polars revisited . Ramsay, Gavin, Cropper, Mark, . MNRAS . 347-497 . 2004 . 2004MNRAS.347..497R ,
Wavelet and R-S analysis of the X-ray flickering of cataclysmic variables . Anzolin, G., Tamburini, F., et all. . A&A . 519-69 . 2010 . 2010A&A...519A..69A ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
The XMM Cluster Survey: X-ray analysis methodology . Lloyd-Davies, E. J., Romer, A. Kathy, et all. . MNRAS . 418-14 . 2011 . 2011MNRAS.418...14L ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . 2012ApJ...756...27L ,
An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2002-03-27T17:04:14Z/2002-04-02T21:07:58Z
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 2003-07-16T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2003-07-16T00:00:00Z, 011125, 17.56_20190403_1200. https://doi.org/10.5270/esa-qxfdshf