LEADER 03325nam 22005415 450 001 9910150551103321 005 20200705143944.0 010 $a4-431-55636-2 024 7 $a10.1007/978-4-431-55636-7 035 $a(CKB)3710000000943847 035 $a(DE-He213)978-4-431-55636-7 035 $a(MiAaPQ)EBC4743120 035 $a(PPN)197138519 035 $a(EXLCZ)993710000000943847 100 $a20161114d2017 u| 0 101 0 $aeng 135 $aurnn|008mamaa 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aShock-Cloud Interaction in RX J1713.7?3946 $eEvidence for Cosmic-Ray Acceleration in the Young VHE ?-ray Supernova Remnant /$fby Hidetoshi Sano 205 $a1st ed. 2017. 210 1$aTokyo :$cSpringer Japan :$cImprint: Springer,$d2017. 215 $a1 online resource (XIII, 134 p. 60 illus., 53 illus. in color.) 225 1 $aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 300 $a"Doctoral Thesis accepted by Nagoya University, Nagoya, Japan." 311 $a4-431-55635-4 320 $aIncludes bibliographical references at the end of each chapters. 327 $aIntroduction -- Non-Thermal X-ray Enhancement around Dense Gas Clumps -- Evidence for the Acceleration of Cosmic Ray Protons -- Evidence for Efficient Acceleration of Cosmic Rays -- Summary and Future Prospects. 330 $aThis book presents a study of the young supernova remnant RX J1713.7-3946 in order to reveal the origin of cosmic rays in our galaxy. The study focuses on the X-ray and gamma radiation from the cosmic ray electrons and protons in the supernova remnant as well as the emission from the surrounding interstellar gas measured by the NANTEN2 4-m radio telescope at Nagoya University. The gamma rays show a good spatial correspondence with the interstellar gas, which for the first time provides strong evidence of the acceleration of cosmic ray protons. Additionally, the author determines that an interaction between the supernova shockwaves and interstellar gas, referred to as ?shock-cloud interaction,? promotes the efficient acceleration of cosmic ray electrons in the supernova remnant. The book reveals that the interstellar gas plays an essential role in producing the high-energy radiation and cosmic rays, offering vital new insights into the origin and behavior of galactic cosmic rays. 410 0$aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 606 $aAstrophysics 606 $aParticle acceleration 606 $aAstrophysics and Astroparticles$3https://scigraph.springernature.com/ontologies/product-market-codes/P22022 606 $aParticle Acceleration and Detection, Beam Physics$3https://scigraph.springernature.com/ontologies/product-market-codes/P23037 615 0$aAstrophysics. 615 0$aParticle acceleration. 615 14$aAstrophysics and Astroparticles. 615 24$aParticle Acceleration and Detection, Beam Physics. 676 $a539.73 700 $aSano$b Hidetoshi$4aut$4http://id.loc.gov/vocabulary/relators/aut$0825093 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910150551103321 996 $aShock-Cloud Interaction in RX J1713.7?3946$91835280 997 $aUNINA