A dataset provided by the European Space Agency

Name: PROBING THE COOLING FLOW IN THE IC 1459 GALAXY GROUP WITH O VII
Published: 2016-11-30T23:00:00Z

Proposal ID	076087
Title	PROBING THE COOLING FLOW IN THE IC 1459 GALAXY GROUP WITH O VII
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0760870101
DOI	https://doi.org/10.5270/esa-q7sdp1d
Principal Investigator, PI	Dr Ciro Pinto
Abstract	We propose to observe the cool (<1 keV) IC 1459 galaxy group with XMM-Newton/RGSfor 120 ks. We will obtain a high quality spectrum with strong O VII-VIII and FeXVII-XVIII emission lines. O VII has never been observed in an individualcluster or group of galaxies until our recent work. These lines will allow us toconstrain the gas cooling rate with high accuracy and to understand the deficitof cool gas in clusters and groups of galaxies and the role of the AGN feedbackin suppressing the cooling flows.
Publications	Insights into the location and dynamics of the coolest X-ray emitting gas in clusters of galaxies \|Pinto C. Fabian A. C. et al. \| MNRAS \| 461-2077 \| 2016 \| 2016MNRAS.461.2077P \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.461.2077P Improved measurements of turbulence in the hot gaseous atmospheres of nearby giant elliptical galaxies \|Ogorzalek A. Zhuravleva I. et al. \| MNRAS \| 472-1659 \| 2017 \| 2017MNRAS.472.1659O \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.472.1659O Correlation between the Total Gravitating Mass of Groups and Clusters and the Supermassive Black Hole Mass of Brightest Galaxies \|Bogdan Akos Lovisari Lorenzo et al. \| ApJ \| 852-131 \| 2018 \| 2018ApJ...852..131B \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...852..131B Black hole mass of central galaxies and cluster mass correlation in cosmological hydro-dynamical simulations \|Bassini L. Rasia E. et al. \| A&A \| 630-144 \| 2019 \| 2019A&A...630A.144B \| http://ui.adsabs.harvard.edu/#abs/2019A&A...630A.144B 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 An XMM-Newton Early-type Galaxy Atlas \|Islam Nazma Kim Dong-Woo et al. \| ApJS \| 256-22 \| 2021 \| 2021ApJS..256...22I \| http://ui.adsabs.harvard.edu/#abs/2021ApJS..256...22I 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 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	2015-11-02T14:05:26Z/2015-11-04T03:33:46Z
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	2016-11-30T23:00:00Z
Last Update	2025-01-27
Keywords	"individual cluster", "ic 1459 galaxy", "cool gas", "quality spectrum", "vii viii", "cooling flow", "xmm newton", "XMM-Newton", "gas cooling rate", "XMM", "cooling flows", "agn feedback"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Ciro Pinto, 2016, 'PROBING THE COOLING FLOW IN THE IC 1459 GALAXY GROUP WITH O VII', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-q7sdp1d