A dataset provided by the European Space Agency

Name 072856
Title Characterizing the periastron environment in the SFXT IGR J16328-4726\r
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0728560201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0728560301

DOI 10.5270/esa-jqn4soh
Author Dr Maria Teresa Fiocchi
Description Investigating the poorly understood accretion mechanism producing the short flares observed from the SFXTs is a key tool in placing these X-ray binaries in the wider context of the HMXBs. Studies of this X-ray binary class are fundamental to understanding the evolution of massive stars, to determining the chemical enrichment of the Galaxy and to give a significant contribution to studying the neutron star equation of the state. Current theories are based on a mass transfer via an isotropic and inhomogeneous clumpy wind or via accretion from anisotropic supergiant wind or on the high magnetic field of neutron stars (>10^14 G) regulating the duration and peak luminosity of the outbursts.Outbursts of IGR J16328-4726 occur at a restricted phase range
Publication The XMM-Newton1 and INTEGRAL2 Observations of the Supergiant Fast X-Ray Transient IGR J16328-4726 . Fiocchi, M., Bazzano, A., et all. . ApJ . 829-125 . 2016 . 2016ApJ...829..125F ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
The accretion environment of supergiant fast X-ray transients probed with XMM-Newton . Bozzo, E., Bernardini, F., et all. . A&A . 608-128 . 2017 . 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 ,
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 all. . MNRAS . 487-420 . 2019 . 2019MNRAS.487..420S ,
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 Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2015-09-19T22:00:00Z, 072856, 17.56_20190403_1200. https://doi.org/10.5270/esa-jqn4soh