A dataset provided by the European Space Agency

Name 020477
Title LARGE MAGELLANIC CLOUD ERNOVA REMNANTS: INVESTIGATION OF EJECTA EMISSION
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0204770101

DOI 10.5270/esa-5l7mnj5
Author Prof KAZIMIERZ BORKOWSKI
Description The detection of ejecta emission in mature supernova remnants can allow the determination of explosion type. This is important for understanding the genesis and evolution of the interstellar medium in galaxies. The Large Magellanic Cloud offers an excellent sample of SNRs at a known distance with little extinction. We propose to observe three remnants in the LMC, 0520-69.4, 0528-69.2, and DEM L241, with XMM-Newton. The spectral resolution of XMM-Newton should allow us to separate reverse shock heated ejecta emission from ISM material heated by the outer blast wave. By performing spatially- resolved spectroscopy on the limb and central regions, our goal is to find evidence of ejecta and determine their chemical composition.
Publication The super-soft source XMMU J052016.0-692505 in the LMC. A likely white dwarf Be-X-ray binary . Kahabka, P., Haberl, F., et all. . A&A . 458-285 . 2006 . 2006A&A...458..285K ,
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Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 2009A&A...496..879M ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
The XMM Cluster Survey: X-ray analysis methodology . Lloyd-Davies, E. J., Romer, A. Kathy, et all. . MNRAS . 418-14 . 2011 . 2011MNRAS.418...14L ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . ...,
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A systematic cross-search for radio-infrared counterparts of XMM- Newton sources . Combi, J. A., Albacete Colombo, J. F., et all. . Ap&SS . 331-53 . 2011 . 2011Ap&SS.331...53C ,
Automatic Classification of Time-variable X-Ray Sources . Lo, Kitty K., Farrell, Sean, et all. . ApJ . 786-20 . 2014 . 2014ApJ...786...20L ,
Spectral and temporal properties of RX J0520.5-6932 (LXP 8.04) during a type-I outburst . Vasilopoulos, G., Haberl, F., et all. . A&A . 567-129 . 2014 . 2014A&A...567A.129V ,
The diversity of quasars unified by accretion and orientation . Shen, Yue, Ho, Luis C., . Natur . 513-210 . 2014 . 2014Natur.513..210S ,
Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters . Xiao, Weike, Chen, Chen, et all. . MNRAS . 432-41 . 2013 . 2013MNRAS.432L..41X ,
The population of X-ray supernova remnants in the Large Magellanic Cloud . Maggi, P., Haberl, F., et all. . A&A . 585-162 . 2016 . 2016A&A...585A.162M ,
The Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo . Miller, Matthew J., Bregman, Joel N., . ApJ . 829-9 . 2016 . 2016ApJ...829....9M ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
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Anisotropy of the galaxy cluster X-ray luminosity-temperature relation . Migkas, Konstantinos, Reiprich, Thomas H., . A&A . 611-50 . 2018 . 2018A&A...611A..50M ,
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X-Ray Luminosity and Size Relationship of Supernova Remnants in the LMC . Ou, Po-Sheng, Chu, You-Hua, et all. . ApJ . 863-137 . 2018 . 2018ApJ...863..137O ,
Testing emergent gravity on galaxy cluster scales . Tamosiunas, Andrius, Bacon, David, et all. . JCAP . 5-53 . 2019 . 2019JCAP...05..053T ,
Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline . Hollowood, Devon L., Jeltema, Tesla, et all. . ApJS . 244-22 . 2019 . 2019ApJS..244...22H ,
Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters . Palmese, A., Annis, J., et all. . MNRAS . 493-4591 . 2020 . 2020MNRAS.493.4591P ,
Mixed-morphology supernova remnants: the case of SNR 0520-69.4 in the Large Magellanic Cloud . Ramu00edrez-Ballinas, I., Reyes-Iturbide, J., et all. . MNRAS . 499-4213 . 2020 . 2020MNRAS.499.4213R ,
New optically identified supernova remnants in the Large Magellanic Cloud . Yew, Miranda, Filipoviu0107, Miroslav D., et all. . MNRAS . 500-2336 . 2021 . 2021MNRAS.500.2336Y ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2004-01-17T20:53:32Z/2004-01-18T07:44:52Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2005-02-15T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2005-02-15T00:00:00Z, 020477, 17.56_20190403_1200. https://doi.org/10.5270/esa-5l7mnj5