A dataset provided by the European Space Agency

Name: The interaction of the supernova remnant Kes 69 with a molecular cloud
Published: 2010-11-14T00:00:00Z

Proposal ID	060548
Title	The interaction of the supernova remnant Kes 69 with a molecular cloud
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605480101
DOI	https://doi.org/10.5270/esa-9rgdqab
Principal Investigator, PI	Dr Marco Miceli
Abstract	We propose to perform a single observation (50 ks) of the mixed-morphologysupernova remnant Kes 69. Recent millimeter-wavelength observations proved thatKes 69 is interacting with a molecular cloud and X-ray emitting knots have beenobserved in the interaction region with ROSAT. Clumps of SNR ejecta moving in adense cloud are predicted to produce a non-thermal knotty emission characterizedby strong lines. This effect has been observed only in IC 443 and with the ROSATdara it is not possible to perform a spatially resolved spectral analysis on theknots in Kes 69. We aim at studying the physical conditions of the plasma in theinteraction region. We will also study the inner part of the remnant toinvestigate the presence of ejecta, recently detected in other mixed-morphology SNRs.
Publications	A population of isolated hard X-ray sources near the supernova remnant Kes 69 \|Bocchino F. Bykov A. M. et al. \| A&A \| 541-152 \| 2012 \| 2012A&A...541A.152B \| http://ui.adsabs.harvard.edu/#abs/2012A&A...541A.152B Detection of X-Ray Periodicity from a New Eclipsing Polar Candidate XGPS-I J183251-100106 \|Hui C. Y. Seo K. A. et al. \| ApJ \| 759-109 \| 2012 \| 2012ApJ...759..109H \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...759..109H Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov V. N. \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y 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 Exploring the Diffuse X-ray Emission of Supernova Remnant Kesteven 69 with XMM-Newton \|Seo Kyoung-Ae Hui Chung Yue \| JASS \| 30-87 \| 2013 \| 2013JASS...30...87S \| http://ui.adsabs.harvard.edu/#abs/2013JASS...30...87S A Suzaku X-ray study of the mixed-morphology supernova remnant Kes 69 and searching for its gamma-ray counterpart \|Sezer A. Ergin T. et al. \| MNRAS \| 481-1416 \| 2018 \| 2018MNRAS.481.1416S \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.481.1416S 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	2009-10-08T23:17:57Z/2009-10-09T16:54:57Z
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	2010-11-14T00:00:00Z
Last Update	2025-01-27
Keywords	"rosat dara", "xray emitting knots", "physical conditions", "dense cloud", "millimeter wavelength", "ic 443", "interaction region", "ROSAT", "resolved spectral analysis", "supernova remnant kes", "molecular cloud"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Marco Miceli, 2010, 'The interaction of the supernova remnant Kes 69 with a molecular cloud', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-9rgdqab