|Title||Large Scale Circumgalactic Coronae around Massive Spiral Galaxies|
|Author||Dr Jiangtao Li|
|Description||Extended coronae around massive spiral galaxies is a key prediction of galaxy formation theory. There are very few such galaxies in the local Universe and even fewer deep X-ray observations of them. We propose to observe 5 luminous, fast rotating, isolated, SF quiescent, and massive spiral galaxies with a total effective exposure of 337ks with XMM-Newton. When combined with archival X-ray observations of 4 other galaxies, the proposal will enable us to compile a mini-sample optimized to constrain the mechanisms responsible for establishing the hot CGM. We will compare radial distributions of coronal properties to the state-of-the-art hydrodynamical simulations, measure the total baryon content, and establish scaling relations of the coronal and other galaxy properties.|
|Publication||XMM-Newton publication statistics . Ness, J.-U., Parmar, A. N., et all. . AN . 335-210 . 2014 . 2014AN....335..210N ,
The Circum-Galactic Medium of MASsive Spirals. I. An Overview and a Case Study of NGC 5908 . Li, Jiang-Tao, Bregman, Joel N., et all. . ApJ . 830-134 . 2016 . 2016ApJ...830..134L ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
The Circum-Galactic Medium of Massive Spirals. II. Probing the Nature of Hot Gaseous Halo around the Most Massive Isolated Spiral Galaxies . Li, Jiang-Tao, Bregman, Joel N., et all. . ApJS . 233-20 . 2017 . 2017ApJS..233...20L ,
Baryon Budget of the Hot Circumgalactic Medium of Massive Spiral Galaxies . Li, Jiang-Tao, Bregman, Joel N., et all. . ApJ . 855-24 . 2018 . 2018ApJ...855L..24L ,
Molecular Gas of the Most Massive Spiral Galaxies. I. A Case Study of NGC 5908 . Li, Jiang-Tao, Zhou, Ping, et all. . ApJ . 877-3 . 2019 . 2019ApJ...877....3L ,
X-ray signatures of black hole feedback: hot galactic atmospheres in IllustrisTNG and X-ray observations . Truong, Nhut, Pillepich, Annalisa, et all. . MNRAS . 494-549 . 2020 . 2020MNRAS.494..549T ,
On the Relation between the Hard X-Ray Photon Index and Accretion Rate for Super-Eddington Accreting Quasars . Huang, Jian, Luo, Bin, et all. . ApJ . 895-114 . 2020 . ...rd.edu/#abs/2020ApJ...895..114H" > 2020ApJ...895..114H ,
|Instrument||EMOS1, EMOS2, EPN, OM, RGS1, RGS2|
|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.
|Publisher And Registrant||European Space Agency|
|Credit Guidelines||European Space Agency, 2016-07-21T22:00:00Z, 074130, 17.56_20190403_1200. https://doi.org/10.5270/esa-z0glf1x|