A dataset provided by the European Space Agency

Name: Probing the disc wind-jet connection in black hole transients II
Published: 2017-10-31T23:00:00Z

Proposal ID	074436
Title	Probing the disc wind-jet connection in black hole transients II
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744361501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744361701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744361801
DOI	https://doi.org/10.5270/esa-txsyz0b
Principal Investigator, PI	Dr Maria Diaz Trigo
Abstract	We propose six observations of one high inclination black hole low mass X-raybinary (LMXB) at different stages of its outburst. We will investigate thepresence of X-ray narrow absorption/emission features in the XMM spectra, whichare a signature of a disc wind, and their relation to the accreting regime. Suchfeatures, identified with ions like FeXXV and FeXXVI, have been observed in anumber of LMXBs and give us information about the mass outflow rate and thelaunching mechanism of the wind. With simultaneous radio observations we willprobe the jet power as a function of the wind properties and how the radio fluxdensity correlates with the X-ray flux at different accretion regimes. We willalso investigate the broadening mechanism of the FeK emission line detected up to now in several LMXBs.
Publications	Simultaneous detection of an intrinsic absorber and a compact jet emission in the X-ray binary IGR J17091-3624 during a hard accretion state \|Gatuzz, E., D\\u00edaz Trigo, M., et al. \| MNRAS \| 491-4857 \| 2020 \| 2020MNRAS.491.4857G \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.491.4857G 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 The current state of disk wind observations in BHLMXBs through X-ray absorption lines in the iron band \|Parra, M., Petrucci, P. -O., et al. \| A&A \| 681-49 \| 2024 \| 2024A&A...681A..49P \| http://ui.adsabs.harvard.edu/#abs/2024A&A...681A..49P 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	2016-03-09T13:38:29Z/2016-03-23T20:55:38Z
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	2017-10-31T23:00:00Z
Keywords	"jet power", "XMM", "accretion regimes", "mass outflow rate", "fek emission line", "xray flux", "broadening mechanism", "xray narrow absorption", "wind properties", "launching mechanism", "xmm spectra", "disc wind", "blackhole transients ii", "accreting regime"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Maria Diaz Trigo, 2017, 'Probing the disc wind-jet connection in black hole transients II', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-txsyz0b