A dataset provided by the European Space Agency

Name: SNR 0534-69.9 and DEM L 316A two Type Ia supernova remnants in the LMC
Published: 2013-03-03T00:00:00Z

Proposal ID	067378
Title	SNR 0534-69.9 and DEM L 316A two Type Ia supernova remnants in the LMC
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673780101
DOI	https://doi.org/10.5270/esa-67kw6ux
Principal Investigator, PI	Dr Daria Kosenko
Abstract	We propose to observe two supernova remnants in the Large Magellanic Cloud(LMC), SNR 0534-69.9 and DEM L 316A, thereby completing the sample of known TypeIa remnants in the LMC observed by XMM-Newton. Our goal is to use the X-rayspectra to measure physical conditions in these SNRs. A detailed analysis of theemission from these objects also provides valuable information on their chemicalstructure, which is linked to the explosion mechanism. We will compare theobserved X-ray spectra with spectra calculated from hydrodynamical models. As asample, the LMC Type Ia remnants will allow us to constrain the parameters ofthermonuclear explosion scenarios.
Publications	The population of X-ray supernova remnants in the Large Magellanic Cloud \|Maggi P. Haberl F. et al. \| A&A \| 585-162 \| 2016 \| 2016A&A...585A.162M \| http://ui.adsabs.harvard.edu/#abs/2016A&A...585A.162M 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 Identification of high-mass X-ray binaries selected from XMM-Newton observations of the LMC* \|van Jaarsveld N. Buckley D. A. H. et al. \| MNRAS \| 475-3253 \| 2018 \| 2018MNRAS.475.3253V \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.475.3253V X-Ray Luminosity and Size Relationship of Supernova Remnants in the LMC \|Ou Po-Sheng Chu You-Hua et al. \| ApJ \| 863-137 \| 2018 \| 2018ApJ...863..137O \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...863..137O New optically identified supernova remnants in the Large Magellanic Cloud \|Yew Miranda Filipoviu0107 Miroslav D. et al. \| MNRAS \| 500-2336 \| 2021 \| 2021MNRAS.500.2336Y \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.500.2336Y 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 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	2012-02-06T00:59:23Z/2012-02-06T18:11:19Z
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	2013-03-03T00:00:00Z
Last Update	2025-01-27
Keywords	"thermonuclear explosion scenarios", "type ia remnant", "physical conditions", "xmm newton", "supernova remnant 0534", "supernova remnant", "XMM-Newton", "explosion mechanism", "thereby completing", "chemical structure", "valuable information", "XMM", "xray spectra", "magellanic cloud lmc", "hydrodynamical models"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Daria Kosenko, 2013, 'SNR 0534-69.9 and DEM L 316A two Type Ia supernova remnants in the LMC', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-67kw6ux