A dataset provided by the European Space Agency

Name: Characterizing the periastron environment in the SFXT IGR J16328-4726
Published: 2015-09-19T22:00:00Z

Proposal ID	072856
Title	Characterizing the periastron environment in the SFXT IGR J16328-4726
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0728560201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0728560301
DOI	https://doi.org/10.5270/esa-jqn4soh
Principal Investigator, PI	Dr Maria Teresa Fiocchi
Abstract	Investigating the poorly understood accretion mechanism producing the shortflares observed from the SFXTs is a key tool in placing these X-ray binaries inthe wider context of the HMXBs. Studies of this X-ray binary class arefundamental to understanding the evolution of massive stars, to determining thechemical enrichment of the Galaxy and to give a significant contribution tostudying the neutron star equation of the state. Current theories are basedon a mass transfer via an isotropic and inhomogeneous clumpy wind or viaaccretion from anisotropic supergiant wind or on the high magnetic field ofneutron stars (>10^14 G) regulating the duration and peak luminosity of theoutbursts.Outbursts of IGR J16328-4726 occur at a restricted phase range
Publications	The XMM-Newton1 and INTEGRAL2 Observations of the Supergiant Fast X-Ray Transient IGR J16328-4726 \|Fiocchi M. Bazzano A. et al. \| ApJ \| 829-125 \| 2016 \| 2016ApJ...829..125F \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829..125F 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 The accretion environment of supergiant fast X-ray transients probed with XMM-Newton \|Bozzo E. Bernardini F. et al. \| A&A \| 608-128 \| 2017 \| 2017A&A...608A.128B \| http://ui.adsabs.harvard.edu/#abs/2017A&A...608A.128B Supergiant fast X-ray transients versus classical supergiant high mass X-ray binaries: Does the difference lie in the companion wind? \|Pradhan P. Bozzo E. \| A&A \| 610-50 \| 2018 \| 2018A&A...610A..50P \| http://ui.adsabs.harvard.edu/#abs/2018A&A...610A..50P Supergiant Fast X-ray Transients uncovered by the EXTraS project: flares reveal the development of magnetospheric instability in accreting neutron stars \|Sidoli Lara Postnov Konstantin A. et al. \| MNRAS \| 487-420 \| 2019 \| 2019MNRAS.487..420S \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.487..420S 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 Statistical Properties of X-Ray Flares from the Supergiant Fast X-Ray Transients \|Zhang Wen-Long Yi Shuang-Xi et al. \| RAA \| 22-65012 \| 2022 \| 2022RAA....22f5012Z \| http://ui.adsabs.harvard.edu/#abs/2022RAA....22f5012Z 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	2014-08-24T19:17:30Z/2014-08-27T01:07:49Z
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	2015-09-19T22:00:00Z
Last Update	2025-01-27
Keywords	"magnetic field", "neutron stars", "short flare", "xray binary", "restricted phase range", "anisotropic supergiant wind", "via accretion", "xray binary class", "wider context", "inhomogeneous clumpy wind", "massive stars", "neutron star equation", "key tool", "chemical enrichment", "peak luminosity", "mass transfer via", "accretion mechanism producing"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Maria Teresa Fiocchi, 2015, 'Characterizing the periastron environment in the SFXT IGR J16328-4726', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-jqn4soh