A dataset provided by the European Space Agency

Name: X-raying the Radio Halo of the Isolated Edge-on Galaxy NGC 3044
Published: 2017-12-22T23:00:00Z

Proposal ID	078265
Title	X-raying the Radio Halo of the Isolated Edge-on Galaxy NGC 3044
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0782650101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0782650201
DOI	https://doi.org/10.5270/esa-8uh2rxo
Principal Investigator, PI	Prof Q. Daniel Wang
Abstract	Cosmic-ray-driven outflows have been suggested to play an essential role ingalaxy formation and evolution. But their relations to galactic coronae andenvironments remain unknown. We propose a deep XMM-Newton observation of theisolated edge-on Sc galaxy NGC 3044, which shows an extended radio halo poweredby galaxy-wide star-forming activity. This observation will enable us to measurethe density structure, as well as the overall extent, morphology,thermal/chemical states of the corona. We will then examine the interplaybetween the corona and cosmic-ray outflows from the galactic disk. The resultswill be compared with those from existing studies of similar galaxies, butmostly undergoing with strong tidal interactions with companions, to explore environmental effects.
Publications	A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies \|Ojha, Vineet, Chand, Hum, et al. \| ApJ \| 896-95 \| 2020 \| 2020ApJ...896...95O \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O 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 A multimission catalogue of ultraluminous X-ray source candidates \|Walton, D. J., Mackenzie, A. D. A., et al. \| MNRAS \| 509-1587 \| 2022 \| 2022MNRAS.509.1587W \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.509.1587W 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 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	2016-12-07T09:33:50Z/2016-12-08T23:49:50Z
Version	PPS_NOT_AVAILABLE
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	2017-12-22T23:00:00Z
Keywords	"tidal interactions", "galactic coronae", "deep xmm newton", "overall extent", "XMM", "cosmic ray outflows", "radio halo powered", "NGC 3044", "galaxy ngc 3044", "galaxy formation", "isolated edge", "XMM-Newton", "x raying", "density structure", "radio halo", "galactic disk", "explore environmental effects"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Q. Daniel Wang, 2017, 'X-raying the Radio Halo of the Isolated Edge-on Galaxy NGC 3044', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-8uh2rxo