Exploring Energy Transfer and Evolution of Supernova Remnants through Year-Scale X-ray Variability / 年単位でのX線時間変動から探る超新星残骸のエネルギー輸送と膨張過程

Description

京都大学 / 新制・課程博士 / 博士(理学) / 甲第25113号 / 理博第5020号 / 新制||理||1716(附属図書館) / 京都大学大学院理学研究科物理学・宇宙物理学専攻 / (主査)教授 鶴 剛, 准教授 榎戸 輝揚, 教授 田島 治 / 学位規則第4条第1項該当 / Doctor of Agricultural Science / Kyoto University / DFAM

Links & Downloads

1. http://hdl.handle.net/2433/288547
2. 10.14989/doctor.k25113
3. 14301

Tags

X-ray Astronomy

Supernova Remnant

Shock Wave

Plasma Physics

Shock Acceleration

400

Additional Fields

Identifer	oai:union.ndltd.org:kyoto-u.ac.jp/oai:repository.kulib.kyoto-u.ac.jp:2433/288547
Date	25 March 2024
Creators	Matsuda, Masamune
Contributors	松田, 真宗, マツダ, マサムネ
Publisher	Kyoto University, 京都大学
Source Sets	Kyoto University
Language	English
Detected Language	English
Type	doctoral thesis, Thesis or Dissertation
Rights	This article has been accepted for publication in Publications of the Astronomical Society of Japan Published by Oxford University Press (DOI: 10.1093/pasj/psaa075). This thesis includes the Accepted Manuscript version of an article accepted for publication in Astrophysical Journal. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at DOI: 10.3847/1538-4357/ac94cf.