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

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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2013-10-11T17:02:05Z/2013-10-12T17:08:45Z
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	2014-10-25T00:00:00Z
Last Update	2025-01-27
Keywords	"spin period", "evolution scenarios", "xmm newton", "magnetic pulsar sxp1062", "XMM-Newton", "neutron star evolution", "neutron star", "powerful tool", "age makes", "accreting neutron stars", "XMM", "accretion powered pulsar", "wind fed hmxb", "key probe", "sxp 1062"
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', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-uvpvn80