A dataset provided by the European Space Agency

Name: G332.5-5.6: An Unusual Supernova Remnant with Circumstellar Interaction
Published: 2011-03-16T00:00:00Z

Proposal ID	060322
Title	G332.5-5.6: An Unusual Supernova Remnant with Circumstellar Interaction
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0603220201
DOI	https://doi.org/10.5270/esa-b9fsve0
Principal Investigator, PI	Dr Kazimierz Borkowski
Abstract	We propose to observe G332.5-5.6, a puzzling supernova remnant with high radiopolarization, central emission with bilaterally symmetric limbs, and evidencefor enhanced nitrogen suggesting interaction with circumstellar material. RecentSuzaku observations of the center show a thermal spectrum with apparent subsolarabundances. Higher angular resolution, coupled with spectroscopy, is required tofollow up this important object and allow the inference of basic SNR propertiessuch as age and shock speed, and to identify any ejecta emission. XMM-Newtonwill image the central emission at ten times higher spatial resolution, andallow a search for morphological structure that can illuminate the spectralanalysis.
Publications	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 An X-ray characterization of the central region of the supernova remnant G332.5-5.6 \|Suarez A. E. Combi J. A. et al. \| A&A \| 583-84 \| 2015 \| 2015A&A...583A..84S \| http://ui.adsabs.harvard.edu/#abs/2015A&A...583A..84S 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 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 The EXTraS project: Exploring the X-ray transient and variable sky \|De Luca A. Salvaterra R. et al. \| A&A \| 650-167 \| 2021 \| 2021A&A...650A.167D \| http://ui.adsabs.harvard.edu/#abs/2021A&A...650A.167D 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	2010-02-20T14:41:30Z/2010-02-21T02:47:14Z
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	2011-03-16T00:00:00Z
Last Update	2025-01-27
Keywords	"thermal spectrum", "ejecta emission", "xmm newton", "central emission", "supernova remnant", "circumstellar interaction", "angular resolution", "enhanced nitrogen", "shock speed", "XMM", "circumstellar material", "radio polarization", "spectral analysis", "XMM-Newton", "apparent subsolar abundance", "G332.5", "bilaterally symmetric limbs", "morphological structure", "spatial resolution"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Kazimierz Borkowski, 2011, 'G332.5-5.6: An Unusual Supernova Remnant with Circumstellar Interaction', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-b9fsve0