A dataset provided by the European Space Agency

Name: W44: Mapping Spectral Morphology with XMM-Newton
Published: 2014-11-15T00:00:00Z

Proposal ID	072163
Title	W44: Mapping Spectral Morphology with XMM-Newton
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721630101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721630201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721630301
DOI	https://doi.org/10.5270/esa-2985a92
Principal Investigator, PI	Dr Randall Smith
Abstract	We propose a 300 ksec observation of the canonical mixed-morphology supernovaremnant (MM SNR) W44, designed to localize and map the recently-discoveredover-ionized plasma via its characteristic radiative recombination continuum andenhanced emission lines. XMM-Newton is the only satellite with the effectivearea and spatial resolution needed to effectively find the origin of this plasmacomponent. These results will be combined with our existing efforts to createthree dimensional magnetohydrodynamic (MHD) models of MM SNR and reveal thesource of this intriguing SNR category that may account for much of theturbulence and triggered star formation in molecular clouds.
Publications	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 Deep XMM-Newton Observations Reveal the Origin of Recombining Plasma in the Supernova Remnant W44 \|Okon Hiromichi Tanaka Takaaki et al. \| ApJ \| 890-62 \| 2020 \| 2020ApJ...890...62O \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...890...62O Recombining plasma in supernova remnants: Discovery and progress in the last decade \|Yamaguchi Hiroya \| AN \| 341-150 \| 2020 \| 2020AN....341..150Y \| http://ui.adsabs.harvard.edu/#abs/2020AN....341..150Y 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	2013-10-18T00:07:22Z/2013-10-24T22:56:05Z
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	2014-11-15T00:00:00Z
Last Update	2025-01-27
Keywords	"triggered star formation", "plasma component", "ionized plasma via", "xmm newton", "mapping spectral morphology", "XMM-Newton", "existing efforts", "XMM", "molecular clouds", "enhanced emission lines", "mm supernova remnant", "spatial resolution"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Randall Smith, 2014, 'W44: Mapping Spectral Morphology with XMM-Newton', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-2985a92