A dataset provided by the European Space Agency

Name: An X-ray exploration of a wind bowshock from a single star
Published: 2011-05-25T00:00:00Z

Proposal ID	065369
Title	An X-ray exploration of a wind bowshock from a single star
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653690101
DOI	https://doi.org/10.5270/esa-0mx73em
Principal Investigator, PI	Mr Victor Zabalza
Abstract	BD+43 3654 is a very massive runaway star likely formed in the central region ofCygnus OB2 association. The interaction of its strong wind with the localinterstellar medium has produced a bow shock that has been detected at theinfrared with the MSX. Multifrequency VLA observations carried out by us show aradio structure clearly correlated with the MSX bow shock and a non-thermalcomponent located at the infrared emission peak position. This indicates that arelativistic population of electrons is present in the shock. This particlepopulation can produce a non-thermal X-ray component, in addition to the thermalcomponent associated with the shocked gas. We propose to detect for the firsttime the X-ray emission from the bow shock produced by a runaway young hot star.
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 X-Ray Observations of Bow Shocks around Runaway O Stars. The Case of zeta Oph and BD+433654 \|Toala J. A. Oskinova L. M. et al. \| ApJ \| 821-79 \| 2016 \| 2016ApJ...821...79T \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...821...79T 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 Search for Diffuse X-Rays from the Bow Shock Region of Runaway Star BD +43 3654 with Suzaku \|Terada Yukikatsu Tashiro Makoto S. et al. \| PASJ \| 64-138 \| 2012 \| 2012PASJ...64..138T \| http://ui.adsabs.harvard.edu/#abs/2012PASJ...64..138T Interferometric Radio Observations of the Interactive Winds of Massive Stars \|Brookes Diane Patricia \| PhDT \| 0-76 \| 2016 \| 2016PhDT........76B \| http://ui.adsabs.harvard.edu/#abs/2016PhDT........76B Multi-zone non-thermal radiative model for stellar bowshocks \|del Palacio S. Bosch-Ramon V. et al. \| A&A \| 617-13 \| 2018 \| 2018A&A...617A..13D \| http://ui.adsabs.harvard.edu/#abs/2018A&A...617A..13D 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 A runaway T Tauri star leaving an extended trail \|Martu00ed Josep Luque-Escamilla Pedro L. \| A&A \| 673-55 \| 2023 \| 2023A&A...673A..55M \| http://ui.adsabs.harvard.edu/#abs/2023A&A...673A..55M Analysis of X-Ray Emission from OB Stars. IV. About X-Ray Emission from Inhomogeneous Winds of OB Stars \|Ryspaeva Elizaveta Kholtygin Alexander \| RAA \| 23-105016 \| 2023 \| 2023RAA....23j5016R \| http://ui.adsabs.harvard.edu/#abs/2023RAA....23j5016R 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	2010-05-08T08:04:21Z/2010-05-08T21:02:56Z
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	2011-05-25T00:00:00Z
Last Update	2025-01-27
Keywords	"radio structure", "bow shock", "central region", "msx bow shock", "local interstellar medium", "hot star", "nonthermal component located", "massive runaway star", "xray emission", "wind bowshock", "particle population", "single star", "cygnus ob2", "multifrequency vla", "nonthermal xray component", "shocked gas", "xray exploration", "relativistic population", "thermal component"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Victor Zabalza, 2011, 'An X-ray exploration of a wind bowshock from a single star', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-0mx73em