A dataset provided by the European Space Agency

Name: Supernova Remnant Evolving in Wind-Blown Bubbles: A Case Study of Kes 27
Published: 2016-04-14T22:00:00Z

Proposal ID	074064
Title	Supernova Remnant Evolving in Wind-Blown Bubbles: A Case Study of Kes 27
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0740640101
DOI	https://doi.org/10.5270/esa-eejea8z
Principal Investigator, PI	Dr Jiangtao Li
Abstract	Mixed-morphology (MM) SNRs represent SN explosion in wind-blown bubbles. Theyare thus good places to study the interaction between massive stellar winds,SNRs, and the surrounding ISM. We propose a 50ks XMM-Newton observation of apeculiar MM SNR, Kes 27. We will map out the spectral parameters in tessellatedmeshes and construct EW maps of some emission lines with our newly developedspatially-resolved spectroscopy method. These analyses will help us tounderstand the unusual properties of this MM SNR, such as the X-ray bright outershell, shell-like interior, and strong NE-SW asymmetry in morphology. We willalso search for evidence of over-ionization state plasma and coherent X-rayfeatures associated with the shell of the HI cavity.
Publications	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 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	2015-03-14T05:12:26Z/2015-03-15T03:25:46Z
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	2016-04-14T22:00:00Z
Keywords	"supernova remnant", "XMM", "spectral parameters", "resolved spectroscopy method", "ne sw asymmetry", "supernova remnant evolving", "massive stellar winds", "tessellated meshes", "mm supernova remnant", "emission lines", "hi cavity", "wind blown bubbles", "XMM-Newton", "construct ew maps", "coherent xray", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Jiangtao Li, 2016, 'Supernova Remnant Evolving in Wind-Blown Bubbles: A Case Study of Kes 27', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-eejea8z