A dataset provided by the European Space Agency

Name: The first full X-ray description of a new young SNR G53.41+0.03
Published: 2021-04-01T00:00:00Z

Proposal ID	084119
Title	The first full X-ray description of a new young SNR G53.41+0.03
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0841190101
DOI	https://doi.org/10.57780/esa-t6dqg7j
Principal Investigator, PI	Mr Vladimir Domcek
Abstract	We propose to obtain the first complete X-ray CCD image of the newly discoveredsupernova remnant (SNR) G53.41+0.03. The spectral image study of this rare andrelatively young (1000 8000 yr) SNR will allow us to\: i) better constraint theelement abundances, which are crucial for pinpointing the SNR origin; ii)significantly improve the age estimation by better measuring the plasmaparameters; iii) search for active acceleration sites producing synchrotronradiation and iv) for a compact object which could be either a normal pulsar,CCO or a magnetar. In addition we will compare the X-ray morphology to ourprevious radio study.
Publications	Completing the X-ray view of the recently discovered supernova remnant G53.41+0.03 \|Dom\\u010dek, V., Vink, J., et al. \| A&A \| 659-63 \| 2022 \| 2022A&A...659A..63D \| http://ui.adsabs.harvard.edu/#abs/2022A&A...659A..63D Energy dependence of quasi-periodic oscillations in accreting X-ray pulsars \|Manikantan, Hemanth, Paul, Biswajit, et al. \| MNRAS \| 531-530 \| 2024 \| 2024MNRAS.531..530M \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.531..530M 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2019-10-13T06:15:27Z/2019-10-14T01:38:47Z
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	2021-04-01T00:00:00Z
Keywords	"G53.41", "iii search", "plasma parameters", "xray morphology", "spectral image", "supernova remnant g53", "element abundance", "compact object", "normal pulsar", "supernova remnant origin"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Vladimir Domcek, 2021, 'The first full X-ray description of a new young SNR G53.41+0.03', 17.56_20190403_1200, European Space Agency, https://doi.org/10.57780/esa-t6dqg7j