A dataset provided by the European Space Agency

Name 065130
Title Follow-up XMM-Newton observations of the cornerstone Wolf-Rayet binary WR140.
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651300301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651300401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651300501

DOI 10.5270/esa-k8s27bv
Author Dr Michael De Becker
Description WR140 is the archetypal long period WR+O colliding wind binary (CWB) system, where the wind from the WR star collides with the wind of its massive companion. Its X-ray brightness, giant IR outbursts, and distinctive non-thermal (NT) radio lightcurve are all attributed to the wind-wind collision region (WCR), the properties of which dramatically change due to the exceptionally high orbital eccentricity (e > 0.88). XMM-Newton observations through periastron passage in AO7 provided unprecedented data on this system. Follow up observations will provide data to complete our view of the X-ray emission from its colliding winds, in order determine the key parameters of this system and the physical processes occuring at the WCR.
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 ,
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 2010-05-08T21:53:30Z/2011-04-06T18:04:08Z
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 2012-04-16T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012-04-16T00:00:00Z, 065130, 17.56_20190403_1200. https://doi.org/10.5270/esa-k8s27bv