A dataset provided by the European Space Agency

Name: Beyond the non-thermal emission of RX J1713.7 3946
Published: 2019-09-11T22:00:00Z

Proposal ID	080430
Title	Beyond the non-thermal emission of RX J1713.7 3946
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804300101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804300301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804300401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804300501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804300601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804300701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804300801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804300901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804301001
DOI	https://doi.org/10.5270/esa-nai97jb
Principal Investigator, PI	Dr Fabio Acero
Abstract	RX J1713.7 3946 is the poster-child of CR accelerator and is among the brightestX- and gamma- ray non-thermal emitters. While the X-ray emission is dominated bysynchrotron, we have revealed thermal emission from the central region of theSNR. This lifted the veil of an unknown aspect of this SNR and preliminaryresults suggests that this might be a common feature. In view of the questionsraised by the recent XMM, Chandra, Fermi, and HESS results, now is the time toundertake a deep X-ray coverage of the entire SNR.
Publications	Progressive steepening of the SNR RX J1713.7-3946 X-ray spectrum from XMM-Newton to INTEGRAL \|Kuznetsova Ekaterina Krivonos Roman et al. \| MNRAS \| 489-1828 \| 2019 \| 2019MNRAS.489.1828K \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.489.1828K X-Ray Hotspots in the Northwest Shell of the Supernova Remnant RX J1713.7-3946 \|Higurashi Ryota Tsuji Naomi \| ApJ \| 899-102 \| 2020 \| 2020ApJ...899..102H \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...899..102H Radial Profiles of Non-thermal Emission from Supernova Remnant RX J1713.7-3946 \|Tang Yunyong Liu Siming \| ApJ \| 909-46 \| 2021 \| 2021ApJ...909...46T \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...909...46T Systematic Study of Acceleration Efficiency in Young Supernova Remnants with Nonthermal X-Ray Observations \|Tsuji Naomi Uchiyama Yasunobu et al. \| ApJ \| 907-117 \| 2021 \| 2021ApJ...907..117T \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907..117T 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 Multiscale multiwavelength extraction of sources and filaments using separation of the structural components: getsf \|Menshchikov A. \| A&A \| 649-89 \| 2021 \| 2021A&A...649A..89M \| http://ui.adsabs.harvard.edu/#abs/2021A&A...649A..89M Pursuing the Origin of the Gamma Rays in RX J1713.7-3946 Quantifying the Hadronic and Leptonic Components \|Fukui Yasuo Sano Hidetoshi et al. \| ApJ \| 915-84 \| 2021 \| 2021ApJ...915...84F \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...915...84F Possible Detection of X-Ray Emitting Circumstellar Material in the Synchrotron-dominated Supernova Remnant RX J1713.7-3946 \|Tateishi Dai Katsuda Satoru et al. \| ApJ \| 923-187 \| 2021 \| 2021ApJ...923..187T \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...923..187T XMM-Newton discovery of very high obscuration in the candidate supergiant fast X-ray transient AX J1714.1-3912 \|Sidoli L. Sguera V. et al. \| MNRAS \| 512-2929 \| 2022 \| 2022MNRAS.512.2929S \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.512.2929S Mapping thermal emission in the synchrotron-dominated supernova remnants G330.2+1.0 3C58 and RX J1713.7-3946 \|Picquenot A. Williams B. J. et al. \| A&A \| 683-A197 \| 2024 \| 2024A&A...683A.197P \| http://ui.adsabs.harvard.edu/#abs/2024A&A...683A.197P The Gamma-Ray Origin of RX J0852.0-4622 Quantifying the Hadronic and Leptonic Components: Further Evidence for the Cosmic-Ray Acceleration in Young Shell-type SNRs \|Fukui Yasuo Aruga Maki et al. \| ApJ \| 961-162 \| 2024 \| 2024ApJ...961..162F \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...961..162F 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	2017-08-29T15:10:48Z/2018-08-27T03:27:59Z
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	2019-09-11T22:00:00Z
Last Update	2025-01-27
Keywords	"poster child", "thermal emission", "J1713.7", "nonthermal emission", "supernova remnant", "deep xray coverage", "xray emission", "cr accelerator", "XMM", "brightest x", "central region", "HESS", "rx j1713"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Fabio Acero, 2019, 'Beyond the non-thermal emission of RX J1713.7 3946', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-nai97jb