id	author	title	date	pages	extension	mime	words	sentence	flesch	summary	cache	txt
app01-2384	Sasaki, Manami	Multi-Wavelength View of Supernova Remnants	2014	6	.pdf	application/pdf	3459	139	63	X-ray synchrotron emission is only observed in younger SNRs and is indicative of electrons with energies of up to 1014 eV. The angular resolution of the newer X-ray tele- scopes, in particular that of the Chandra X-ray obser- vatory, made it possible to reveal narrow filaments of non-thermal X-ray emission close to the outer shock in several young SNRs: Soon after, more SNRs were also confirmed to radiate non-thermal X-ray emission: Cas A (e.g., The et al., 1996, Allen et al., 1997), RX J1713.7-3946 (G347.3- 0.5, Pfeffermann & Aschenbach, 1996), RX J0852.0- 4622 (G266.2-1.2, Vela Jr, Aschenbach 1998).	cache/app01-2384.pdf	txt/app01-2384.txt