A dataset provided by the European Space Agency

Name 076087
Title PROBING THE COOLING FLOW IN THE IC 1459 GALAXY GROUP WITH O VII
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0760870101

DOI 10.5270/esa-q7sdp1d
Author Dr Ciro Pinto
Description We propose to observe the cool (<1 keV) IC 1459 galaxy group with XMM-Newton-RGS for 120 ks. We will obtain a high quality spectrum with strong O VII-VIII and Fe XVII-XVIII emission lines. O VII has never been observed in an individual cluster or group of galaxies until our recent work. These lines will allow us to constrain the gas cooling rate with high accuracy and to understand the deficit of cool gas in clusters and groups of galaxies and the role of the AGN feedback in suppressing the cooling flows.
Publication Insights into the location and dynamics of the coolest X-ray emitting gas in clusters of galaxies . Pinto, C., Fabian, A. C., et all. . MNRAS . 461-2077 . 2016 . 2016MNRAS.461.2077P ,
Improved measurements of turbulence in the hot gaseous atmospheres of nearby giant elliptical galaxies . Ogorzalek, A., Zhuravleva, I., et all. . MNRAS . 472-1659 . 2017 . 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 all. . ApJ . 852-131 . 2018 . 2018ApJ...852..131B ,
Black hole mass of central galaxies and cluster mass correlation in cosmological hydro-dynamical simulations . Bassini, L., Rasia, E., et all. . A&A . 630-144 . 2019 . 2019A&A...630A.144B ,
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 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 2016-11-30T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2016-11-30T23:00:00Z, 076087, 17.56_20190403_1200. https://doi.org/10.5270/esa-q7sdp1d