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  1. 010 学術雑誌論文
  2. 池内, 了 / IKEUCHI, Satoru

Evolution of Supernova Remnants. 1. Interacting Supernova Remnants

https://ir.soken.ac.jp/records/3313
https://ir.soken.ac.jp/records/3313
451855ca-28b2-46c4-82b6-24c22d81ee27
Item type 学術雑誌論文 / Journal Article(1)
公開日 2013-01-09
タイトル
タイトル Evolution of Supernova Remnants. 1. Interacting Supernova Remnants
タイトル
タイトル Evolution of Supernova Remnants. 1. Interacting Supernova Remnants
言語 en
言語
言語 eng
キーワード
言語 en
主題Scheme Other
主題 Interstellar matter,Shock waves,Supernova remnants,X-rays
資源タイプ
資源タイプ識別子 http://purl.org/coar/resource_type/c_6501
資源タイプ journal article
アクセス権
アクセス権 metadata only access
アクセス権URI http://purl.org/coar/access_right/c_14cb
著者 IKEUCHI, Satoru

× IKEUCHI, Satoru

IKEUCHI, Satoru

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著者別名 池内, 了

× 池内, 了

池内, 了

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抄録
内容記述タイプ Abstract
内容記述 The evolution and structure of two interacting supernova remnants
(SNRS) are calculated by use of a timedependent two-dimensional hydro-
dynamic code. The interactions of two SNRs are simulated in such a
Way that at a time t。 after the first supernova explosion, the second
Supernova explosion occurs at the distance D and two SNRs encounter.
Two cases are investigated; the second explosion occurs outside or in-
Side the expanding she11 0f the first SNR.I n the first case, the final
Structures of two interacting SNRs are typica11y classified into three
types:(1) two SNRs merge into a single-1ike SNR,(2) two SNRs merge
but show a peanut-shape structure, and (3) two SNRs do not merge.1n
the second case, they reduce to two types:(1) Two SNRs evolve as an
isolated SNR with twice the explosion energy, and (2) in the she11 of the
first SNR a bump is formed due to the shock impact by the second ex-
Plosion. The critical distances for the above structural changes are
examined, as we11 as the changes ot the expansion law trom an isolated
SNR. With these results some discussions are given on the formation
of an SNR tunnel system and the possibility of gas ejection from a
galaxy. Based upon this view' of interacting SNRS, a preliminary model
for the solar neighborhood and loop l is presented.
書誌情報 Publications of the Astronomical Society of Japan
en : Publications of the Astronomical Society of Japan

巻 30, p. 563-580, 発行日 1978-10
出版者
出版者 The Astronomical Society of Japan
ISSN
収録物識別子タイプ ISSN
収録物識別子 00046264
権利
権利情報 © The Astronomical Society of Japan
関連サイト
識別子タイプ URI
関連識別子 http://pasj.asj.or.jp/info/subscription.html
関連名称 Copyright
関連サイト
識別子タイプ URI
関連識別子 http://adsabs.harvard.edu/full/1978PASJ...30..563I%7CCited
関連名称 The Astronomical Society of Japan
フォーマット
内容記述タイプ Other
内容記述 application/pdf
著者版フラグ
出版タイプ VoR
出版タイプResource http://purl.org/coar/version/c_970fb48d4fbd8a85
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