A dataset provided by the European Space Agency

Name 001854
Title Colliding Wind X-ray Emission in the LBV Binary HD 5980
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0018540101

DOI 10.5270/esa-63qb81n
Author Dr Michael Corcoran
Description HD 5980 is a massive binary in the SMC which underwent a unique Luminous Blue Variable-type eruption in 1994. X-ray emission arises from the collision of the 2 winds from the component stars, and possibly from interaction of the material ejected during the eruption with the ISM and-or stellar winds. XMM-EPIC observations will be used to characterize the wind speeds and to constrain the masses and radii of the stellar components, the total amount of material ejected in the eruption, and the chemical composition of the stellar winds
Publication First Detection of Phase-dependent Colliding Wind X-Ray Emission outside the Milky Way . Naze, Yael, Corcoran, Michael F., et all. . ApJ . 658-25 . 2007 . 2007ApJ...658L..25N ,
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 ,
X-ray spectra from magnetar candidates - III. Fitting SGR-AXP soft X-ray emission with non-relativistic Monte Carlo models . Zane, S., Rea, N., et all. . MNRAS . 398-1403 . 2009 . 2009MNRAS.398.1403Z ,
XMM-Newton observations of the Small Magellanic Cloud: the 280 s Be-X-ray binary pulsar AX J0058-7203 in outburst . Haberl, F., Pietsch, W., . A&A . 476-317 . 2007 . 2007A&A...476..317H ,
XMM-Newton observations of the Small Magellanic Cloud: Long term evolution of frequently observed Be-X-ray binaries . Eger, P., Haberl, F., . A&A . 491-841 . 2008 . 2008A&A...491..841E ,
Addendum: ''Discovery of a Possible Anomalous X-Ray Pulsar in the Small Magellanic Cloud.. (ApJ, 574, L29 ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-11-20T23:36:11Z/2001-11-21T07:16:29Z
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 2003-02-17T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2003-02-17T00:00:00Z, 001854, 17.56_20190403_1200. https://doi.org/10.5270/esa-63qb81n