A dataset provided by the European Space Agency

Name: Spatially Resolved X-ray Spectrsocopy of the Wind-Blown Bubble NGC 2359
Published: 2014-04-18T00:00:00Z

Proposal ID	069039
Title	Spatially Resolved X-ray Spectrsocopy of the Wind-Blown Bubble NGC 2359
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690390101
DOI	https://doi.org/10.5270/esa-eg7pqoh
Principal Investigator, PI	Dr Svetozar ZHEKOV
Abstract	Fast winds from massive stars create large cavities in the surroundinginterstellar medium filled with hot gas, known as Wind-Blown Bubbles (WBB). Wepropose to obtain EPIC imaging spectroscopy of the WBB NGC 2359. Thanks to theEPIC excellent sensitivity, we will: (i) obtain a high quality CCD spectrumwhich can be used to constrain the temperature of the hot plasma and theefficiency of thermal conduction across the bubble wall, (ii) determine thespatial distribution and properties of X-ray emitting plasma, (iii) test andrefine shock physics models of WBB by a direct confrontation of their resultswith observations; (iv) study the X-ray properties of the presumably single WRstar WR 7.
Publications	X-rays from wind-blown bubbles: an XMM-Newton detection of NGC 2359 \|Zhekov Svetozar A. \| MNRAS \| 443-12 \| 2014 \| 2014MNRAS.443...12Z \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.443...12Z On the diffuse X-ray emission from the Wolf-Rayet bubble NGC 2359 \|Toala J. A. Guerrero M. A. et al. \| MNRAS \| 446-1083 \| 2015 \| 2015MNRAS.446.1083T \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.446.1083T The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F 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 Multiple variability time-scales of the early nitrogen-rich Wolf-Rayet star WR 7 \|Toalu00e1 J. A. Bowman D. M. et al. \| MNRAS \| 514-2269 \| 2022 \| 2022MNRAS.514.2269T \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.514.2269T 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	RGS1, EPN, RGS2, EMOS1, OM, EMOS2
Temporal Coverage	2013-04-09T13:34:52Z/2013-04-10T20:26:47Z
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	2014-04-18T00:00:00Z
Last Update	2025-01-27
Keywords	"spatial distribution", "NGC 2359", "interstellar medium filled", "EPIC", "quality ccd spectrum", "massive stars create", "epic imaging spectroscopy", "xray properties", "resolved xray spectrsocopy", "wbb ngc 2359", "hot plasma", "thermal conduction", "fast winds", "bubble wall", "xray emitting plasma", "iii test", "hot gas"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Svetozar ZHEKOV, 2014, 'Spatially Resolved X-ray Spectrsocopy of the Wind-Blown Bubble NGC 2359', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-eg7pqoh