Proposal ID | 078208 |
Title | THE RARE CASE OF SNR G346.6-0.2: THE NON-THERMAL MIXED-MORPHOLOGY SNR |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0782080101 |
DOI | https://doi.org/10.5270/esa-06hlro9 |
Principal Investigator, PI | Dr Katie Auchettl |
Abstract | The detection of non-thermal X-ray emission from supernovas remnants (SNRs)provides us a unique window to study particle acceleration at their shock-front.All of the ~14 SNRs in which non-thermal X-ray synchrotron emission has beendetected are shell-like in nature, and show no evidence of interaction withlarge nearby molecular clouds. We propose a deep XMM and NuSTAR observation ofSNR G346.6-0.2, which is a rare case of a molecular cloud interacting,mixed-morphology SNR that shows non-thermal X-ray emission. These observationswill allow us to constrain and characterise the power-law tail, better definethe thermal X-ray properties across the remnant, determine the effect that adense environment has these properties, as well as the plasma conditions which lead to nonthermal X-rays. |
Publications |
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Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2016-09-04T16:07:23Z/2016-09-05T23:14:02Z |
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 | 2017-09-23T22:00:00Z |
Keywords | "NuSTAR", "nonthermal xray emission", "supernova remnant g346", "supernova remnant", "shock front", "power law tail", "thermal xray properties", "XMM", "molecular cloud interacting", "nearby molecular clouds", "deep xmm", "G346.6", "nonthermal xray", "particle acceleration", "plasma conditions" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Dr Katie Auchettl, 2017, 'THE RARE CASE OF SNR G346.6-0.2: THE NON-THERMAL MIXED-MORPHOLOGY SNR', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-06hlro9 |