A dataset provided by the European Space Agency

Name: AN ACCRETION DISK WIND AT LOW EDDINGTON RATE
Published: 2017-09-30T22:00:00Z

Proposal ID	079078
Title	AN ACCRETION DISK WIND AT LOW EDDINGTON RATE
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0790780101
DOI	https://doi.org/10.5270/esa-6me8ylf
Principal Investigator, PI	Dr Nathalie Degenaar
Abstract	According to the current paradigm, accretion onto black holes and neutron starsis associated with two types of outflows that are mutually exclusive. At >E-2 ofthe Eddington limit, disk winds are detected through narrow X-ray absorptionfeatures, whereas at lower mass-accretion rates radio jets are seen. However,our AO1 NuSTAR observation of the neutron star low-mass X-ray binary IGRJ17062-6143 revealed a virgul3-4 sigma narrow absorption line at virgul6.85 keV. Thisprovides the very first evidence that disk winds can be launched at merely virgulE-3of Eddington, and may co-exist with a radio jet. We propose for a 75 ks NuSTARobservation and a supporting 70 ks XMM observation to solidify this measurement,which would change our current views of inflow-outflow coupling in accreting compact objects.
Publications	The very faint X-ray binary IGR J17062-6143: a truncated disc, no pulsations, and a possible outflow \|van den Eijnden, J., Degenaar, N., et al. \| MNRAS \| 475-2027 \| 2018 \| 2018MNRAS.475.2027V \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.475.2027V Multiwavelength characterization of the accreting millisecond X-ray pulsar and ultracompact binary IGR J17062-6143 \|Hern\\u00e1ndez Santisteban, J. V., C\\u00faneo, V., et al. \| MNRAS \| 488-4596 \| 2019 \| 2019MNRAS.488.4596H \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.488.4596H The chemical composition of the accretion disc and donor star in ultra-compact X-ray binaries: A comprehensive X-ray analysis \|Koliopanos, Filippos, P\\u00e9ault, Mathias, et al. \| MNRAS \| 501-548 \| 2021 \| 2021MNRAS.501..548K \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.501..548K 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 Long-term Coherent Timing of the Accreting Millisecond Pulsar IGR J17062-6143 \|Bult, Peter, Strohmayer, Tod E., et al. \| ApJ \| 912-120 \| 2021 \| 2021ApJ...912..120B \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...912..120B The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions \|Pan, Zeyang, Qu, Zhijie, et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P 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	2016-09-13T12:03:52Z/2016-09-14T06:05:32Z
Version	19.17_20220121_1250
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	2017-09-30T22:00:00Z
Keywords	"NuSTAR", "neutron stars", "low eddington rate", "XMM", "eddington limit", "mutually exclusive", "radio jet", "inflow outflow coupling", "85 kev", "narrow xray absorption", "co exist", "75 nustar", "accretion disk wind", "disk winds", "ao1 nustar", "accreting compact objects"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Nathalie Degenaar, 2017, 'AN ACCRETION DISK WIND AT LOW EDDINGTON RATE', 19.17_20220121_1250, European Space Agency, https://doi.org/10.5270/esa-6me8ylf