A dataset provided by the European Space Agency

Name 015309
Title HU Aqr: A magnetic accretion key study
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0153090101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0153090201

DOI 10.5270/esa-uhr79nq
Author Dr Axel Schwope
Description HU Aqr is a unique, bright eclipsing polar (AM Herculis binary) providing incredible diagnostic power at X-ray and optical wavelengths. This includes eclipses by the mass-donating companion star, pre-eclipse dips caused by absorption in the accretion stream, and selfeclipses of the accretion spot by the white dwarf. Previous ROSAT-EUVE-optical observations resolved (marginally) the accretion spot, revealed a strongly evolving light curve and displayed a large scatter in eclipse timings. With XMM-Newton we will monitor the spectral evolution of the source, study the interaction of the accretion stream with the magnetosphere and measure the location and size of the accretion spot in soft and hard X-rays as a function of mass transfer rate with unprecedented accuracy.
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 ,
Hunting high and low: XMM monitoring of the eclipsing polar HU Aquarii . Schwarz, R., Schwope, A. D., et all. . A&A . 496-833 . 2009 . 2009A&A...496..833S ,
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 and O VIII Emission Intensities . Henley, David B., Shelton, Robin L., . ApJS . 202-14 . 2012 . 2012ApJS..202...14H ,
The...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2003-05-20T10:11:51Z/2003-10-25T02:55:36Z
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 2004-11-20T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004-11-20T00:00:00Z, 015309, 17.56_20190403_1200. https://doi.org/10.5270/esa-uhr79nq