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Proposal ID 030713
Title An XMM Study of SNRs Discovered with the Canadian Galactic Plane Survey
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0307130101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0307130201
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DOI https://doi.org/10.5270/esa-7cxrele
Principal Investigator, PI Prof Samar Safi-Harb
Abstract Increasing the sample of neutron star-SNR associations is needed to study thedynamics and evolution of supernova explosions of massive stars and to unveilthe properties of their collapsed cores. Four young low-surface brightness SNRswere recently discovered with the Canadian Galactic Plane Survey. All four SNRsare believed to be the remnants of core-collapse explosions, young, and harborROSAT or Chandra point sources. We here propose to observe these SNRs withXMM-Newton in order to primarily detect and characterize their X-ray emission.Their low-surface brightness, high column density, size, age, and lack of X-rayspectral information, make XMM the best satellite to date to perform this study.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2005-05-31T10:12:34Z/2005-11-25T05:30:48Z
Version 21.51_20241115_1113
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 2006-12-15T00:00:00Z
Last Update 2026-07-09
Keywords "massive stars", "core collapse explosions", "ROSAT", "XMM-Newton", "xray spectral information", "collapsed cores", "harbor rosat", "low surface brightness", "supernova remnant", "XMM", "xray emission", "supernova explosions", "column density", "xmm newton"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Prof Samar Safi-Harb, 2006, 'An XMM Study of SNRs Discovered with the Canadian Galactic Plane Survey', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-7cxrele
Rights Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.