A dataset provided by the European Space Agency

Name: The Structure of the Bow Shock Nebula Surrounding PSR B1853+01 in the SNR W44
Published: 2010-05-20T00:00:00Z

Proposal ID	055106
Title	The Structure of the Bow Shock Nebula Surrounding PSR B1853+01 in the SNR W44
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551060101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551060201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551060301
DOI	https://doi.org/10.5270/esa-o1xalmq
Principal Investigator, PI	Dr Robert Petre
Abstract	The pulsar wind bow shock nebula surrounding PSR B1853+01, embedded within theSNR W44, is the oldest known wind nebula associated with an active pulsar.Chandra observations have shown that the X-ray morphology is that of anasymmetric nebula trailing behind the pulsar.s apparent motion direction, with asmaller extent than the radio. A recent, deep Chandra image suggests an extendedregion of emission preceding the pulsar. The verification of the nature of thisemission as nonthermal and associated with the pulsar has strong implicationsfor our understanding of pulsar bow shock nebulae. We propose a 75 ks EPICobservation of this intriguing object, exploiting XMM-Newton.s unique surfacebrightness sensitivity above 3 keV to establish the nature of the emission.
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 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 Exploring the end states of massive stars using the X-ray emission of neutron stars and supernova remnants \|Prinz, Tobias, \| PhDT \| 0-305 \| 2013 \| 2013PhDT.......305P \| http://ui.adsabs.harvard.edu/#abs/2013PhDT.......305P Deep XMM-Newton Observations Reveal the Origin of Recombining Plasma in the Supernova Remnant W44 \|Okon, Hiromichi, Tanaka, Takaaki, et al. \| ApJ \| 890-62 \| 2020 \| 2020ApJ...890...62O \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...890...62O Recombining plasma in supernova remnants: Discovery and progress in the last decade \|Yamaguchi, Hiroya, \| AN \| 341-150 \| 2020 \| 2020AN....341..150Y \| http://ui.adsabs.harvard.edu/#abs/2020AN....341..150Y 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	2009-04-24T09:57:06Z/2009-04-25T10:26:07Z
Version	PPS_NOT_AVAILABLE
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	2010-05-20T00:00:00Z
Keywords	"active pulsar", "bow shock nebula", "asymmetric nebula trailing", "intriguing object", "XMM", "exploiting xmm newton", "supernova remnant w44", "deep chandra image", "wind nebula", "75 epic", "emission preceding", "xray morphology", "surface brightness sensitivity", "apparent motion direction", "psr b1853", "XMM-Newton", "EPIC"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Robert Petre, 2010, 'The Structure of the Bow Shock Nebula Surrounding PSR B1853+01 in the SNR W44', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-o1xalmq