{"_buckets": {"deposit": "fe7c1e54-ca66-43a4-a027-058233c79764"}, "_deposit": {"created_by": 21, "id": "3294", "owners": [21], "pid": {"revision_id": 0, "type": "depid", "value": "3294"}, "status": "published"}, "_oai": {"id": "oai:ir.soken.ac.jp:00003294", "sets": ["274"]}, "author_link": ["750", "754", "752", "743", "745", "744", "734", "746", "751", "748", "753", "749", "738", "747"], "item_10001_biblio_info_7": {"attribute_name": "書誌情報", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2003-10", "bibliographicIssueDateType": "Issued"}, "bibliographicIssueNumber": "5", "bibliographicPageEnd": "L64", "bibliographicPageStart": "L61", "bibliographicVolumeNumber": "55", "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": "Supernova remnants ( = SNR) are suggested to be sites of cosmic-ray acceleration. In particular, it has been an issue of keen interest whether cosmic ray protons are being accelerated in a SNR which emits TeV γ-rays. A crucial observational test for this is to find dense molecular gas towards the SNR, because such molecular gas can best verify the existence of cosmic-ray protons via pion decay to γ-rays. Here, we show that new high-resolution mm-wave observations of interstellar CO molecule have revealed molecular gas at 1kpc distance interacting with the TeV γ-ray SNR G 347.3 - 0.5, and that a molecular cloud of ˜ 200 solar masses is clearly associated with the TeV γ-ray peak, providing strong evidence for proton acceleration. We have estimated the total energy of accelerated protons to be ˜ 1048 erg, which corresponds to an acceleration efficiency of ˜ 0.001, posing an observational constraint on the proton acceleration. ", "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_14": {"attribute_name": "DOI", "attribute_value_mlt": [{"subitem_relation_name": [{"subitem_relation_name_text": "10.1093/pasj/55.5.L61"}], "subitem_relation_type": "isIdenticalTo", "subitem_relation_type_id": {"subitem_relation_type_id_text": "https://doi.org/10.1093/pasj/55.5.L61", "subitem_relation_type_select": "DOI"}}]}, "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"}}]}, "item_10001_rights_15": {"attribute_name": "権利", "attribute_value_mlt": [{"subitem_rights": "\u0001© 2003. 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_creator": {"attribute_name": "著者", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "FUKUI, Yasuo"}], "nameIdentifiers": [{"nameIdentifier": "743", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "MORIGUCHI, Yoshiaki"}], "nameIdentifiers": [{"nameIdentifier": "744", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "TAMURA, Keisuke"}], "nameIdentifiers": [{"nameIdentifier": "745", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "YAMAMOTO, Hiroaki"}], "nameIdentifiers": [{"nameIdentifier": "746", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "TAWARA, Yuzuru"}], "nameIdentifiers": [{"nameIdentifier": "747", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "MIZUNO, Norikazu"}], "nameIdentifiers": [{"nameIdentifier": "748", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "ONISHI, Toshikazu"}], "nameIdentifiers": [{"nameIdentifier": "749", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "MIZUNO, Akira"}], "nameIdentifiers": [{"nameIdentifier": "750", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "UCHIYAMA, Yasunobu"}], "nameIdentifiers": [{"nameIdentifier": "751", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "HIRAGA, Junko"}], "nameIdentifiers": [{"nameIdentifier": "752", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "TAKAHASHI, Tadayuki"}], "nameIdentifiers": [{"nameIdentifier": "753", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "YAMASHITA, Koujin"}], "nameIdentifiers": [{"nameIdentifier": "754", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "IKEUCHI, Satoru"}], "nameIdentifiers": [{"nameIdentifier": "734", "nameIdentifierScheme": "WEKO"}]}]}, "item_files": {"attribute_name": "ファイル情報", "attribute_type": "file", "attribute_value_mlt": [{"accessrole": "open_date", "date": [{"dateType": "Available", "dateValue": "2012-12-17"}], "displaytype": "simple", "download_preview_message": "", "file_order": 0, "filename": "55052495.pdf", "filesize": [{"value": "432.0 kB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_11", "mimetype": "application/pdf", "size": 432000.0, "url": {"label": "55052495", "url": "https://ir.soken.ac.jp/record/3294/files/55052495.pdf"}, "version_id": "aaba90f1-1ba6-4ee7-b18b-6f625a7d1fe8"}]}, "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": "Discovery of Interacting Molecular Gas toward the TeV Gamma-Ray Peak of the SNR G 347.3-0.5", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "Discovery of Interacting Molecular Gas toward the TeV Gamma-Ray Peak of the SNR G 347.3-0.5"}, {"subitem_title": "Discovery of Interacting Molecular Gas toward the TeV Gamma-Ray Peak of the SNR G 347.3-0.5", "subitem_title_language": "en"}]}, "item_type_id": "10001", "owner": "21", "path": ["95", "274"], "permalink_uri": "https://ir.soken.ac.jp/records/3294", "pubdate": {"attribute_name": "公開日", "attribute_value": "2012-12-13"}, "publish_date": "2012-12-13", "publish_status": "0", "recid": "3294", "relation": {}, "relation_version_is_last": true, "title": ["Discovery of Interacting Molecular Gas toward the TeV Gamma-Ray Peak of the SNR G 347.3-0.5"], "weko_shared_id": 21}