A dataset provided by the European Space Agency

Name: The enigma of the magnetic pulsar SXP1062: a new look with XMM-Newton
Published: 2014-10-25T00:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	072196
Title	The enigma of the magnetic pulsar SXP1062: a new look with XMM-Newton
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721960101
DOI	https://doi.org/10.5270/esa-uvpvn80
Principal Investigator, PI	Dr Lidia Oskinova
Abstract	SXP 1062 is an exceptional case of a young neutron star with known age in awind-fed HMXB. A unique combination of measured spin period, its derivative,luminosity and young age makes this source a key probe for the physics ofaccretion and neutron star evolution. All current accretion scenarios encountermajor difficulties explaining the spin-down rate of this accretion-poweredpulsar. This study will allow us to construct a spin period-luminosity relationas a powerful tool for distinguishing between different accretion and evolutionscenarios. The XMM-Newton observations of SXP 1062 will thus shed new light onthe physics of accreting neutron stars.
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 Comprehensive Library of X-Ray Pulsars in the Small Magellanic Cloud: Time Evolution of Their Luminosities and Spin Periods \|Yang J. Laycock S. G. T. et al. \| ApJ \| 839-119 \| 2017 \| 2017ApJ...839..119Y \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...839..119Y Discovery of a glitch in the accretion-powered pulsar SXP 1062 \|Serim M. M. Sahiner S. et al. \| MNRAS \| 471-4982 \| 2017 \| 2017MNRAS.471.4982S \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.471.4982S A multiwavelength study of SXP 1062 the long-period X-ray pulsar associated with a supernova remnant \|Gonzalez-Galan A. Oskinova L. M. et al. \| MNRAS \| 475-2809 \| 2018 \| 2018MNRAS.475.2809G \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.475.2809G Identification of AGN in the XMM-Newton X-ray survey of the SMC \|Maitra Chandreyee Haberl Frank et al. \| A&A \| 622-29 \| 2019 \| 2019A&A...622A..29M \| http://ui.adsabs.harvard.edu/#abs/2019A&A...622A..29M The supernova remnant population of the Small Magellanic Cloud \|Maggi Pierre Filipoviu0107 Miroslav D. et al. \| A&A \| 631-127 \| 2019 \| 2019A&A...631A.127M \| http://ui.adsabs.harvard.edu/#abs/2019A&A...631A.127M On the Geometry of the X-ray emission from pulsars a consistent inclination and beaming solution for the Be/X-ray pulsar SXP 1062 \|Cappallo R. C. Laycock S. G. T. et al. \| MNRAS \| 495-2152 \| 2020 \| 2020MNRAS.495.2152C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.495.2152C 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 Spitzer and Herschel studies of dust in supernova remnants in the Small Magellanic Cloud \|Matsuura Mikako Ayley Victoria et al. \| MNRAS \| 513-1154 \| 2022 \| 2022MNRAS.513.1154M \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.513.1154M 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 Pulse timing studies of X-ray binaries: GX 1+4 Swift J0513.4- 6547 X Persei and SXP 1062 \|Serim Muhammed Mirau00e7 \| PhDT \| 0-222 \| 2019 \| 2019PhDT.......222S \| http://ui.adsabs.harvard.edu/#abs/2019PhDT.......222S 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	2013-10-11T17:02:05Z/2013-10-12T17:08:45Z
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	2014-10-25T00:00:00Z
Last Update	2026-06-19
Keywords	"powerful tool", "accretion powered pulsar", "age makes", "neutron star evolution", "neutron star", "XMM", "accreting neutron stars", "magnetic pulsar sxp1062", "xmm newton", "evolution scenarios", "spin period", "XMM-Newton", "sxp 1062", "key probe", "wind fed hmxb"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Lidia Oskinova, 2014, 'The enigma of the magnetic pulsar SXP1062: a new look with XMM-Newton', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-uvpvn80
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.