A dataset provided by the European Space Agency

Name: Measuring the shock speed in RX J1713.7-3946
Published: 2016-04-01T22:00:00Z

Proposal ID	074303
Title	Measuring the shock speed in RX J1713.7-3946
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743030101
DOI	https://doi.org/10.5270/esa-hzsbi3u
Principal Investigator, PI	Dr Fabio Acero
Abstract	These expansion measurements are a powerful way to probe the basic, but oftenunknown, parameters of the SNR such as age, distance and ambient medium densityin which the shock is expanding. In particular, determining the ambient densityis a crucial parameter for constraining the fraction of kinetic energytransferred to hadrons accelerated at the front shock of the SNR. In theprototypical accelerator RX J1713.7-3946, no thermal X-ray emission (from theshocked medium) has been observed and proper motion measurement is probably thebest way to constrain the ambient density.
Publications	Measurement of the X-ray proper motion in the south-east rim of RX J1713.7-3946 \|Acero, Fabio, Katsuda, Satoru, et al. \| A&A \| 597-106 \| 2017 \| 2017A&A...597A.106A \| http://ui.adsabs.harvard.edu/#abs/2017A&A...597A.106A 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 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 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 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 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	2015-03-10T21:36:40Z/2015-03-11T20:55:00Z
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	2016-04-01T22:00:00Z
Keywords	"ambient density", "J1713.7", "thermal xray emission", "supernova remnant", "expansion measurements", "rx j1713", "front shock", "ambient medium density", "hadrons accelerated", "shocked medium", "kinetic energy transferred", "shock speed", "proper motion measurement"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Fabio Acero, 2016, 'Measuring the shock speed in RX J1713.7-3946', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-hzsbi3u