{"_buckets": {"deposit": "870091c5-df0b-4b7a-b596-5eb24b2728a5"}, "_deposit": {"created_by": 21, "id": "3313", "owners": [21], "pid": {"revision_id": 0, "type": "depid", "value": "3313"}, "status": "published"}, "_oai": {"id": "oai:ir.soken.ac.jp:00003313", "sets": ["274"]}, "author_link": ["734", "738"], "item_10001_biblio_info_7": {"attribute_name": "書誌情報", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "1978-10", "bibliographicIssueDateType": "Issued"}, "bibliographicPageEnd": "580", "bibliographicPageStart": "563", "bibliographicVolumeNumber": "30", "bibliographic_titles": [{"bibliographic_title": "Publications of the Astronomical Society of Japan"}, {"bibliographic_title": "Publications of the Astronomical Society of Japan", "bibliographic_titleLang": "en"}]}]}, "item_10001_creator_3": {"attribute_name": "著者別名", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "池内, 了"}], "nameIdentifiers": [{"nameIdentifier": "738", "nameIdentifierScheme": "WEKO"}, {"nameIdentifier": "1000090025461", "nameIdentifierScheme": "NRID", "nameIdentifierURI": " "}, {"nameIdentifier": "90025461", "nameIdentifierScheme": "e-Rad", "nameIdentifierURI": "https://kaken.nii.ac.jp/ja/search/?qm=90025461"}]}]}, "item_10001_description_19": {"attribute_name": "フォーマット", "attribute_value_mlt": [{"subitem_description": "application/pdf", "subitem_description_type": "Other"}]}, "item_10001_description_5": {"attribute_name": "抄録", "attribute_value_mlt": [{"subitem_description": "The evolution and structure of two interacting supernova remnants\n(SNRS) are calculated by use of a timedependent two-dimensional hydro-\ndynamic code. The interactions of two SNRs are simulated in such a\nWay that at a time t。 after the first supernova explosion, the second\nSupernova explosion occurs at the distance D and two SNRs encounter.\nTwo cases are investigated; the second explosion occurs outside or in-\nSide the expanding she11 0f the first SNR.I n the first case, the final\nStructures of two interacting SNRs are typica11y classified into three\ntypes:(1) two SNRs merge into a single-1ike SNR,(2) two SNRs merge\nbut show a peanut-shape structure, and (3) two SNRs do not merge.1n\nthe second case, they reduce to two types:(1) Two SNRs evolve as an\nisolated SNR with twice the explosion energy, and (2) in the she11 of the\nfirst SNR a bump is formed due to the shock impact by the second ex-\nPlosion. The critical distances for the above structural changes are\nexamined, as we11 as the changes ot the expansion law trom an isolated\nSNR. With these results some discussions are given on the formation\nof an SNR tunnel system and the possibility of gas ejection from a\ngalaxy. Based upon this view\u0027 of interacting SNRS, a preliminary model\nfor the solar neighborhood and loop l is presented.\n", "subitem_description_type": "Abstract"}]}, "item_10001_publisher_8": {"attribute_name": "出版者", "attribute_value_mlt": [{"subitem_publisher": "The Astronomical Society of Japan"}]}, "item_10001_relation_17": {"attribute_name": "関連サイト", "attribute_value_mlt": [{"subitem_relation_name": [{"subitem_relation_name_text": "Copyright"}], "subitem_relation_type_id": {"subitem_relation_type_id_text": "http://pasj.asj.or.jp/info/subscription.html", "subitem_relation_type_select": "URI"}}, {"subitem_relation_name": [{"subitem_relation_name_text": "The Astronomical Society of Japan"}], "subitem_relation_type_id": {"subitem_relation_type_id_text": "http://adsabs.harvard.edu/full/1978PASJ...30..563I%7CCited", "subitem_relation_type_select": "URI"}}]}, "item_10001_rights_15": {"attribute_name": "権利", "attribute_value_mlt": [{"subitem_rights": "© The Astronomical Society of Japan"}]}, "item_10001_source_id_9": {"attribute_name": "ISSN", "attribute_value_mlt": [{"subitem_source_identifier": "00046264 ", "subitem_source_identifier_type": "ISSN"}]}, "item_10001_version_type_20": {"attribute_name": "著者版フラグ", "attribute_value_mlt": [{"subitem_version_resource": "http://purl.org/coar/version/c_970fb48d4fbd8a85", "subitem_version_type": "VoR"}]}, "item_access_right": {"attribute_name": "アクセス権", "attribute_value_mlt": [{"subitem_access_right": "metadata only access", "subitem_access_right_uri": "http://purl.org/coar/access_right/c_14cb"}]}, "item_creator": {"attribute_name": "著者", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "IKEUCHI, Satoru"}], "nameIdentifiers": [{"nameIdentifier": "734", "nameIdentifierScheme": "WEKO"}]}]}, "item_keyword": {"attribute_name": "キーワード", "attribute_value_mlt": [{"subitem_subject": "Interstellar matter,Shock waves,Supernova remnants,X-rays", "subitem_subject_language": "en", "subitem_subject_scheme": "Other"}]}, "item_language": {"attribute_name": "言語", "attribute_value_mlt": [{"subitem_language": "eng"}]}, "item_resource_type": {"attribute_name": "資源タイプ", "attribute_value_mlt": [{"resourcetype": "journal article", "resourceuri": "http://purl.org/coar/resource_type/c_6501"}]}, "item_title": "Evolution of Supernova Remnants. 1. Interacting Supernova Remnants", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "Evolution of Supernova Remnants. 1. Interacting Supernova Remnants"}, {"subitem_title": "Evolution of Supernova Remnants. 1. Interacting Supernova Remnants", "subitem_title_language": "en"}]}, "item_type_id": "10001", "owner": "21", "path": ["95", "274"], "permalink_uri": "https://ir.soken.ac.jp/records/3313", "pubdate": {"attribute_name": "公開日", "attribute_value": "2013-01-09"}, "publish_date": "2013-01-09", "publish_status": "0", "recid": "3313", "relation": {}, "relation_version_is_last": true, "title": ["Evolution of Supernova Remnants. 1. Interacting Supernova Remnants"], "weko_shared_id": 21}