A dataset provided by the European Space Agency

Name: Non-thermal X-rays from bow shock runaways: a legacy programme for XMM-Newton
Published: 2016-04-14T22:00:00Z

Proposal ID	074366
Title	Non-thermal X-rays from bow shock runaways: a legacy programme for XMM-Newton
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743660101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743660201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743660301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743660401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743660501
DOI	https://doi.org/10.5270/esa-65c4vdi
Principal Investigator, PI	Dr Michael De Becker
Abstract	Massive stars ejected from their birth place, the so-called runaway massivestars, are likely to produce strong bow shocks through the interaction of thetheir stellar winds with the interstellar medium. Such shocks have been provento be efficient at accelerating particles, as revealed by the identification ofnon-thermal radiation in a couple of objects. This large programme aims atobtaining measurements of the non-thermal X-ray flux of a carefully selectedsample of bow shock runaways (BSRs), to quantify their capability to accelerateparticles, in relation with their potential contribution to the production ofGalactic cosmic-rays. Such an unprecedented collection of data is aimed atconstituting some kind of legacy programme for XMM-Newton, before the advent of future generation X-ray observatories.
Publications	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 On the Absence of Non-thermal X-Ray Emission around Runaway O Stars \|Toala J. A. Oskinova L. M. \| ApJ \| 838-19 \| 2017 \| 2017ApJ...838L..19T \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...838L..19T X-ray study of bow shocks in runaway stars \|De Becker M. del Valle M. V. et al. \| MNRAS \| 471-4452 \| 2017 \| 2017MNRAS.471.4452D \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.471.4452D Is the Pollocks paradigm of X-ray emission for O stars correct? \|Ryspaeva E. B. Kholtygin A. F. \| AN \| 338-959 \| 2017 \| 2017AN....338..959R \| http://ui.adsabs.harvard.edu/#abs/2017AN....338..959R The long-period massive binary HD 54662 revisited \|Mossoux E. Mahy L. \| A&A \| 615-19 \| 2018 \| 2018A&A...615A..19M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...615A..19M Analysis of the X-ray emission of OB stars: O stars \|Ryspaeva Elizaveta Kholtygin Alexander \| RAA \| 18-104 \| 2018 \| 2018RAA....18..104R \| http://ui.adsabs.harvard.edu/#abs/2018RAA....18..104R Analysis of the X-ray emission of OB stars II: B stars \|Ryspaeva Elizaveta Kholtygin Alexander \| RAA \| 19-120 \| 2019 \| 2019RAA....19..120R \| http://ui.adsabs.harvard.edu/#abs/2019RAA....19..120R 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 The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions \|Pan Zeyang Qu Zhijie et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P 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	2014-10-01T17:16:20Z/2015-03-16T16:33:34Z
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	2016-04-14T22:00:00Z
Last Update	2025-01-27
Keywords	"galactic cosmic rays", "interstellar medium", "accelerating particles", "nonthermal xray", "xmm newton", "XMM-Newton", "accelerate particles", "programme aims", "nonthermal radiation", "massive stars", "XMM", "stellar winds", "nonthermal xray flux", "bow shock runaways", "bow shoc"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Michael De Becker, 2016, 'Non-thermal X-rays from bow shock runaways: a legacy programme for XMM-Newton', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-65c4vdi