A dataset provided by the European Space Agency

Name: AGN Feedback in Action: the powerful wind in IRAS F05054+1718
Published: 2022-10-08T00:00:00Z

Proposal ID	089068
Title	AGN Feedback in Action: the powerful wind in IRAS F05054+1718
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0890680101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0890680201
DOI	https://doi.org/10.57780/esa-mgc5m7m
Principal Investigator, PI	Dr Valentina Braito
Abstract	We propose simultaneous NuSTAR (80 ksec) & XMM-Newton (60 ksec) observations ofIRASF05054+1718, a local (z = 0.0175) Seyfert 2 galaxy, which hosts a powerfuldisk wind and where there is evidence of quenching of star formation. In thissource, Swift data suggested the presence of a powerful and high-velocity (vouta?? 0.1 c) wind, most likely launched within 100Rg . A short NuSTAR observationconfirms the presence of such a wind, but with a much higher velocity (vout a??0.2 c). Neither of the two previous observations have the statistical qualityneeded to fully investigate the physical properties of this wind. Our aim hereis to confirm the disk wind at a higher statistical significance.
Publications	Another X-ray UFO without a momentum-boosted molecular outflow. ALMA CO(1-0) observations of the galaxy pair IRAS 05054+1718 \|Bonanomi Francesca Cicone Claudia et al. \| A&A \| 673-46 \| 2023 \| 2023A&A...673A..46B \| http://ui.adsabs.harvard.edu/#abs/2023A&A...673A..46B 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2021-09-11T11:23:24Z/2021-09-12T07:59:13Z
Version	19.16_20210326_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	2022-10-08T00:00:00Z
Last Update	2025-08-04
Keywords	"XMM", "0175 seyfert", "XMM-Newton", "NuSTAR", "disk wind", "physical properties", "iras f05054", "agn feedback", "velocity vout", "xmm newton", "statistical significance", "statistical quality", "star formation", "short nustar", "powerful wind", "swift data suggested", "powerful disk wind", "local z"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Valentina Braito, 2022, 'AGN Feedback in Action: the powerful wind in IRAS F05054+1718', 19.16_20210326_1200, European Space Agency, https://doi.org/10.57780/esa-mgc5m7m