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  1. B100 理学部/理学研究科
  2. B100d 学位論文
  3. 博士論文(理博・論理博)

G109.1-1.0: A Supernova Remnant Interacting with a Molecular Cloud : 分子雲と相互作用する超新星残骸G109.1-1.0

http://hdl.handle.net/2237/12579
http://hdl.handle.net/2237/12579
7164d1c0-1a52-4c8b-bef3-603cab14b1c3
名前 / ファイル ライセンス アクション
ko2042_abstr.pdf ko2042_abstr.pdf (144.1 kB)
ko2042.pdf ko2042.pdf (2.8 MB)
Item type 学位論文 / Thesis or Dissertation(1)
公開日 2009-12-28
タイトル
タイトル G109.1-1.0: A Supernova Remnant Interacting with a Molecular Cloud : 分子雲と相互作用する超新星残骸G109.1-1.0
言語 en
著者 立松, 健一

× 立松, 健一

WEKO 32287

ja 立松, 健一

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Tatematsu, Kenichi

× Tatematsu, Kenichi

WEKO 32288

en Tatematsu, Kenichi

Search repository
アクセス権
アクセス権 open access
アクセス権URI http://purl.org/coar/access_right/c_abf2
抄録
内容記述 The molecular cloud in the vicinity of the peculiar supernova remnant G1O9.1-1.0 has been observed in the J =1-0 transitions or CO molecules. The Nagoya 4 m radio telescope and the Nobeyama 45 m radio telescope were used for the observations. It is found that the main molecular cloud on the west has prevented an isotropic expansion of G1O9.1-1.0 Causing its semicircular shape of this remnant. The CO arm extending from the main molecular cloud shows an apparent anticorrelation with the curled X-ray feature seen in G1O9.1-1.0 called the X-ray jetlike feature. The CO arm is round to consist or two thin CO filaments. At least one of these filaments should be located near the rear remnant shell. Molecules which were located in a thin (<0.5 pc) original surface layer of the molecular cloud are thought to have been fully dissociated due to the SNR shock. It is expected that the momentum deposited in the cloud shock will compress the molecular cloud to some extent in 10^5-10^6 yr. The X-ray jetlike feature probably represents the density distribution of the hot plasma in this SNR. Three explanations for this feature are proposed, and there is a possibility that the existence or the molecular cloud has contributed to the formation or this feature. The present observations have clearly revealed that G1O9.1-1.0 accompanies the molecular cloud and that they interact with each other.
言語 en
内容記述タイプ Abstract
内容記述
内容記述 名古屋大学博士学位論文 学位の種類 : 理学博士(課程) 学位授与年月日 : 昭和63年3月25日
言語 ja
内容記述タイプ Other
言語
言語 eng
資源タイプ
資源 http://purl.org/coar/resource_type/c_db06
タイプ doctoral thesis
書誌情報
発行日 1988-03-25
学位名
言語 ja
学位名 理学博士
学位授与機関
学位授与機関識別子Scheme kakenhi
学位授与機関識別子 13901
言語 ja
学位授与機関名 名古屋大学
言語 en
学位授与機関名 Nagoya University
学位授与年度
学位授与年度 1987
学位授与年月日
学位授与年月日 1988-03-25
学位授与番号
学位授与番号 甲第2042号
フォーマット
application/pdf
フォーマット
application/pdf
著者版フラグ
値 publisher
URI
識別子 http://hdl.handle.net/2237/12579
識別子タイプ HDL
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