A dataset provided by the European Space Agency

Name: PSR B1929+10 - the most serious challenge for electron acceleration in a PWN
Published: 2014-04-27T00:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	069520
Title	PSR B1929+10 - the most serious challenge for electron acceleration in a PWN
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0695200101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0695200201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0695200301
DOI	https://doi.org/10.5270/esa-q22wghq
Principal Investigator, PI	Prof Werner Becker
Abstract	XMM-Newton has confirmed the existence of the diffuse X-ray emission with atrail morphology lying in a direction opposite to the transverse motion of themillion year old pulsar PSR B1929+10. A possible interpretation of the emissionis that it is a synchrotron wake from particles left behind by the pulsar as itmoves through the ISM. We propose deep spectro-imaging observations of thepulsars X-ray trail with XMM-Newton in order to explore the emission processesat work and to measure its length/width and spectral evolution as a function ofdistance from the pulsar.
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 A deep X-ray spectral imaging of the bow-shock pulsar wind nebula associated with PSR B1929+10 \|Kim S. I. Hui C. Y. et al. \| A&A \| 637-7 \| 2020 \| 2020A&A...637L...7K \| http://ui.adsabs.harvard.edu/#abs/2020A&A...637L...7K 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 Dynamical Response of Solar Wind Charge Exchange Soft X-Ray Emission in Earths Magnetosphere to the Solar Wind Proton Flux \|Zhang Yingjie Sun Tianran et al. \| ApJ \| 948-69 \| 2023 \| 2023ApJ...948...69Z \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...948...69Z Extreme accretion events: TDEs and changingu2011look AGN \|Komossa S. Grupe D. \| AN \| 344-20230015 \| 2023 \| 2023AN....34430015K \| http://ui.adsabs.harvard.edu/#abs/2023AN....34430015K 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 New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2013-03-30T12:28:50Z/2013-04-14T20:19:30Z
Version	21.51_20241115_1113
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	2014-04-27T00:00:00Z
Last Update	2026-07-09
Keywords	"deep spectro imaging", "XMM-Newton", "xray trail", "synchrotron wake", "spectral evolution", "trail morphology lying", "direction opposite", "electron acceleration", "XMM", "transverse motion", "emission processes", "pulsar psr b1929", "psr b1929", "particles left", "diffuse xray emission", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Werner Becker, 2014, 'PSR B1929+10 - the most serious challenge for electron acceleration in a PWN', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-q22wghq
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.