|Title||XMM-Newton observation of the dust-making Wolf-Rayet star WR106|
|Author||Dr Michael De Becker|
|Description||The issue of the X-ray emission from Wolf-Rayet (WR) stars is far from being elucidated. Thanks to previous observations, we know indeed that even though several WN-type WR are detected in X-rays, it appears that single WC stars are not detected, most probably because of the strong opacity of the stellar wind. However, significant X-ray emission is expected if WC stars are part of a colliding-wind binary system. In the case of dust-making WR stars (WC-type with dense stellar winds), dust is most probably produced in a wind-wind interaction region. Performed and forthcoming interferometric observations in the near-infrared (VLTI, PI: De Becker) will help us to investigate the multiplicity of WR106.(abridged)|
|Publication||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 ,
Tentative insight into the multiplicity of the persistent dust maker WR 106 from X-ray observations . De Becker, M., . NewA . 41-5 . 2015 . 2015NewA...41....5D ,
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|
|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.
|Publisher And Registrant||European Space Agency|
|Credit Guidelines||European Space Agency, 2013-09-28T00:00:00Z, 069081, 17.56_20190403_1200. https://doi.org/10.5270/esa-3dt2dl7|