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
License: https://creativecommons.org/licenses/by-nc/3.0/igo

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 Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE \|Ma Xiangyao Zhang Yanxia et al. \| AJ \| 168-210 \| 2024 \| 2024AJ....168..210M \| http://ui.adsabs.harvard.edu/#abs/2024AJ....168..210M New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D CHANG-ES XXXIu2014A Decade of CHANG-ES: What We Have Learned from Radio Observations of Edge-on Galaxies \|Irwin Judith Beck Rainer et al. \| Galax \| 12-22 \| 2024 \| 2024Galax..12...22I \| http://ui.adsabs.harvard.edu/#abs/2024Galax..12...22I
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
Last Update	2026-07-09
Keywords	"tidal interactions", "galactic disk", "x raying", "overall extent", "XMM-Newton", "NGC 3044", "radio halo", "cosmic ray outflows", "isolated edge", "galaxy ngc 3044", "explore environmental effects", "galaxy formation", "XMM", "galactic coronae", "radio halo powered", "deep xmm newton", "density structure"
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
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.