A dataset provided by the European Space Agency

Name: Exploring the halo around an extremely massive comma jet launching spiral galaxy
Published: 2019-01-15T23:00:00Z

Proposal ID	080063
Title	Exploring the halo around an extremely massive, jet launching spiral galaxy
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800630101
DOI	https://doi.org/10.5270/esa-a5p56w4
Principal Investigator, PI	Dr Stephen Walker
Abstract	Here we propose to observe the extremely massive, rapidly rotating, relativisticjet launching, spiral galaxy 2MASX J23453268-0449256 for 85ks to observe its hothalo, measure its mass content and map its morphology. It is extremely rare fora massive spiral galaxy to eject relativistic jets, as they are nearly alwayslaunched from the nuclei of bulge dominated ellipticals and not flat spirals. Itis clear that J2345-0449 is an extremely rare system whose properties challengethe standard paradigm for the formation of relativistic jets in AGN. DetailedX-ray observations are necessary to understand this system and complement theexcellent HST, Gemini, GMRT and VLA data.
Publications	Exploring the hot gaseous halo around an extremely massive and relativistic jet launching spiral galaxy with XMM-Newton \|Mirakhor, M. S., Walker, S. A., et al. \| MNRAS \| 500-2503 \| 2021 \| 2021MNRAS.500.2503M \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.500.2503M 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 Dynamical Response of Solar Wind Charge Exchange Soft X-Ray Emission in Earth.s Magnetosphere to the Solar Wind Proton Flux \|Zhang, Yingjie, Sun, Tianran, et al. \| ApJ \| 948-69 \| 2023 \| 2023ApJ...948...69Z \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...948...69Z 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	2017-12-19T07:53:48Z/2017-12-20T11:32:08Z
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	2019-01-15T23:00:00Z
Keywords	"relativistic jet launching", "bulge dominated ellipticals", "eject relativistic jets", "hot halo", "relativistic jets", "standard paradigm", "vla data", "massive spiral galaxy", "rare system", "j2345 0449", "mass content", "HST", "flat spirals"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Stephen Walker, 2019, 'Exploring the halo around an extremely massive comma jet launching spiral galaxy', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-a5p56w4