東華大學圖書館 |

語系: 繁體中文

說明(常見問題)

回圖書館首頁

手機版館藏查詢

登入

回首頁 到查詢結果 [ subject:"Supernova remnants." ]

切換: 標籤 | MARC模式 | ISBD

Shock-cloud interaction in RX J1713....

Sano, Hidetoshi.

FindBook

Google Book

Amazon

博客來

Shock-cloud interaction in RX J1713.7-3946 = evidence for cosmic-ray acceleration in the Young Vhe [gamma]-ray supernova remnant /

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	Shock-cloud interaction in RX J1713.7-3946/ by Hidetoshi Sano.
其他題名:	evidence for cosmic-ray acceleration in the Young Vhe [gamma]-ray supernova remnant /
作者:	Sano, Hidetoshi.
出版者:	Tokyo :Springer Japan : : 2017.,
面頁冊數:	xiii, 134 p. :ill. (some col.), digital ;24 cm.
內容註:	Introduction -- 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.
Contained By:	Springer eBooks
標題:	Cosmic rays. -
電子資源:	http://dx.doi.org/10.1007/978-4-431-55636-7
ISBN:	9784431556367

Shock-cloud interaction in RX J1713.7-3946 = evidence for cosmic-ray acceleration in the Young Vhe [gamma]-ray supernova remnant /
Sano, Hidetoshi.

Shock-cloud interaction in RX J1713.7-3946evidence for cosmic-ray acceleration in the Young Vhe [gamma]-ray supernova remnant /[electronic resource] :by Hidetoshi Sano. - Tokyo :Springer Japan :2017. - xiii, 134 p. :ill. (some col.), digital ;24 cm. - Springer theses,2190-5053. - Springer theses..

Introduction -- 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.

This 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.

ISBN: 9784431556367

Standard No.: 10.1007/978-4-431-55636-7doiSubjects--Topical Terms:

836138
Cosmic rays.

LC Class. No.: QC485

Dewey Class. No.: 523.019

Shock-cloud interaction in RX J1713.7-3946 = evidence for cosmic-ray acceleration in the Young Vhe [gamma]-ray supernova remnant /
LDR:02265nmm a2200325 a 4500 001 2088793
003 DE-He213
005 20161114142353.0
006 m d
007 cr nn 008maaau
008 171013s2017 ja s 0 eng d
020 $a 9784431556367 $q (electronic bk.)
020 $a 9784431556350 $q (paper)
024 7 $a 10.1007/978-4-431-55636-7 $2 doi
035 $a 978-4-431-55636-7
040 $a GP $c GP
041 0 $a eng
050 4 $a QC485
072 7 $a PHVB $2 bicssc
072 7 $a SCI005000 $2 bisacsh
082 0 4 $a 523.019 $2 23
090 $a QC485 $b .S228 2017
100 1 $a Sano, Hidetoshi. $3 3218835
245 1 0 $a Shock-cloud interaction in RX J1713.7-3946 $h [electronic resource] : $b evidence for cosmic-ray acceleration in the Young Vhe [gamma]-ray supernova remnant / $c by Hidetoshi Sano.
260 $a Tokyo : $b Springer Japan : $b Imprint: Springer, $c 2017.
300 $a xiii, 134 p. : $b ill. (some col.), digital ; $c 24 cm.
490 1 $a Springer theses, $x 2190-5053
505 0 $a Introduction -- 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.
520 $a This 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.
650 0 $a Cosmic rays. $3 836138
650 0 $a Supernova remnants. $3 3218836
650 1 4 $a Physics. $3 516296
650 2 4 $a Astrophysics and Astroparticles. $3 1067087
650 2 4 $a Particle acceleration and detection, Beam Physics. $3 2180493
710 2 $a SpringerLink (Online service) $3 836513
773 0 $t Springer eBooks
830 0 $a Springer theses. $3 1314442
856 4 0 $u http://dx.doi.org/10.1007/978-4-431-55636-7
950 $a Physics and Astronomy (Springer-11651)