A dataset provided by the European Space Agency

Name: The Wind-Wind Interaction Region and Stellar Wind Geometry of V444 Cyg
Published: 2013-07-06T00:00:00Z

Proposal ID	069281
Title	The Wind-Wind Interaction Region and Stellar Wind Geometry of V444 Cyg
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0692810301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0692810401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0692810501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0692810601
DOI	https://doi.org/10.5270/esa-yzg1qo2
Principal Investigator, PI	Ms Jamie Lomax
Abstract	Angular momentum and mass loss from massive binary star systems is poorlyconstrained; however, eclipsing colliding-wind systems provide usefullaboratories in which to study these processes. V444 Cyg is a bright, WN5+O6colliding-wind system that shows different eclipse behaviors in the hard andsoft X-rays. We ask for XMM-Newton observations that, combined with opticalspectropolarimetric observations, will significantly improve our understandingof the 3D structure of the winds and wind-wind collision region in V444 Cyg.
Publications	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 \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y V444 Cygni X-ray and polarimetric variability: Radiative and Coriolis forces shape the wind collision region \|Lomax J. R. Naze Y. et al. \| A&A \| 573-43 \| 2015 \| 2015A&A...573A..43L \| http://ui.adsabs.harvard.edu/#abs/2015A&A...573A..43L The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F Classification of 4XMM-DR9 sources by machine learning \|Zhang Yanxia Zhao Yongheng \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2012-05-05T20:43:34Z/2012-06-15T04:45:44Z
Version	17.56_20190403_1200
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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	2013-07-06T00:00:00Z
Last Update	2025-01-27
Keywords	"eclipse behaviors", "stellar wind geometry", "mass loss", "xmm newton", "XMM-Newton", "optical spectropolarimetric", "poorly constrained", "soft xray", "XMM", "v444 cyg", "useful laboratories", "3d structure", "angular momentum"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Ms Jamie Lomax, 2013, 'The Wind-Wind Interaction Region and Stellar Wind Geometry of V444 Cyg', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-yzg1qo2