A dataset provided by the European Space Agency

Name: Multiwavelength observations of PSR B1259-63 periastron passage in 2010-2011
Published: 2012-03-30T00:00:00Z

Proposal ID	065364
Title	Multiwavelength observations of PSR B1259-63 periastron passage in 2010-2011
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653640401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653640501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653640601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653640701
DOI	https://doi.org/10.5270/esa-addyqdm
Principal Investigator, PI	Prof Andrii Neronov
Abstract	PSR B1259-63 is a unique binary system with a radio pulsar from which unpulsedX-ray, gamma-ray, and radio emission was observed. The pulsar is in a highlyeccentric 3.4 year orbit around a Be star. Collision of the pulsar wind with thewind of Be star plays a crucial role in generation of the observed emission. Thegoal of this proposal is to investigate, for the first time, simultaneous X-ray(XMM-Newton) and GeV gamma-ray (Fermi) spectral evolution of the system as thepulsar passes through the Be star disk. Details of the X-ray/gamma-ray spectralevolution will allow to probe the physical mechanism(s) of particle accelerationand interactions during collision of relativistic pulsar wind with the wind fromthe massive star.
Publications	Multiwavelength observations of the binary system PSR B1259-63/LS 2883 around the 2010-2011 periastron passage \|Chernyakova M. Abdo A. A. et al. \| MNRAS \| 439-432 \| 2014 \| 2014MNRAS.439..432C \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.439..432C 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 NuSTAR Discovery of an Unusually Steady Long-term Spin-up of the Be Binary 2RXP J130159.6-635806 \|Krivonos Roman A. Tsygankov Sergey S. et al. \| ApJ \| 809-140 \| 2015 \| 2015ApJ...809..140K \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...809..140K Multi-wavelength observations of the binary system PSR B1259-63/LS 2883 around the 2014 periastron passage \|Chernyakova M. Neronov A. et al. \| MNRAS \| 454-1358 \| 2015 \| 2015MNRAS.454.1358C \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.454.1358C 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 Observational and theoretical study of the point sources of very high energy gamma-ray emission \|Babyk Iurii \| PhDT \| 0-5 \| 2017 \| 2017PhDT.........5B \| http://ui.adsabs.harvard.edu/#abs/2017PhDT.........5B Spectroscopic identification of INTEGRAL high-energy sources with VLT/ISAAC \|Fortin F. Chaty S. et al. \| A&A \| 618-150 \| 2018 \| 2018A&A...618A.150F \| http://ui.adsabs.harvard.edu/#abs/2018A&A...618A.150F Modelling multiwavelength emissions from PSR B1259-63/LS 2883: Effects of the stellar disc on shock radiations \|Chen A. M. Takata J. et al. \| A&A \| 627-87 \| 2019 \| 2019A&A...627A..87C \| http://ui.adsabs.harvard.edu/#abs/2019A&A...627A..87C 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	2011-01-06T14:48:16Z/2011-03-04T09:34:22Z
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	2012-03-30T00:00:00Z
Last Update	2025-01-27
Keywords	"radio pulsar", "periastron passage", "massive star", "xray xmm newton", "binary system", "XMM", "psr b1259", "physical mechanisms", "radio emission", "particle acceleration", "star disk", "pulsar wind", "pulsar passes", "XMM-Newton", "relativistic pulsar wind", "2010 2011", "star plays", "unpulsed xray", "gamma ray"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Andrii Neronov, 2012, 'Multiwavelength observations of PSR B1259-63 periastron passage in 2010-2011', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-addyqdm