WEKO3
アイテム
{"_buckets": {"deposit": "84c1d337-a950-4332-99d1-4f9930532a10"}, "_deposit": {"created_by": 18, "id": "9099", "owners": [18], "pid": {"revision_id": 0, "type": "depid", "value": "9099"}, "status": "published"}, "_oai": {"id": "oai:ir.kagoshima-u.ac.jp:00009099", "sets": []}, "author_link": ["115028", "115029", "115030", "115031", "115032", "115033", "115034", "115035"], "item_6_biblio_info_5": {"attribute_name": "収録雑誌名", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2012", "bibliographicIssueDateType": "Issued"}, "bibliographicIssueNumber": "5", "bibliographicPageStart": "98", "bibliographicVolumeNumber": "64", "bibliographic_titles": [{"bibliographic_title": "Publications of the Astronomical Society of Japan", "bibliographic_titleLang": "en"}]}]}, "item_6_date_6": {"attribute_name": "作成日", "attribute_value_mlt": [{"subitem_date_issued_datetime": "2012-10-25", "subitem_date_issued_type": "Issued"}]}, "item_6_description_4": {"attribute_name": "要約(Abstract)", "attribute_value_mlt": [{"subitem_description": "We observed four \"water fountain\" sources in the CO J = 3→2 line emission with the Atacama Submillimeter Telescope Experiment (ASTE) 10m telescope in 2010–2011. The water fountain sources are evolved stars that form high-velocity collimated jets traced by H2O maser emission. The CO line was detected only from IRAS 16342-3814. The present work confirmed that the 12CO to 13CO line intensity ratio is ~1.5 at the systemic velocity. We discuss the origins of the very low 12CO-to-13CO intensity ratio, as possible evidence for \"hot-bottom burning\" in an oxygen-rich star, and the CO intensity variation in IRAS 16342-3814.", "subitem_description_language": "en", "subitem_description_type": "Other"}]}, "item_6_publisher_23": {"attribute_name": "公開者・出版者", "attribute_value_mlt": [{"subitem_publisher": "Astronomical Society of Japan", "subitem_publisher_language": "en"}, {"subitem_publisher": "日本天文学会", "subitem_publisher_language": "ja"}]}, "item_6_relation_11": {"attribute_name": "DOI", "attribute_value_mlt": [{"subitem_relation_type": "isIdenticalTo", "subitem_relation_type_id": {"subitem_relation_type_id_text": "https://doi.org/10.1093/pasj/64.5.98", "subitem_relation_type_select": "DOI"}}]}, "item_6_rights_12": {"attribute_name": "権利", "attribute_value_mlt": [{"subitem_rights": "Astronomical Society of Japan", "subitem_rights_language": "en"}]}, "item_6_source_id_7": {"attribute_name": "ISSN", "attribute_value_mlt": [{"subitem_source_identifier": "00046264", "subitem_source_identifier_type": "PISSN"}]}, "item_6_source_id_9": {"attribute_name": "NII書誌ID", "attribute_value_mlt": [{"subitem_source_identifier": "AA1082896X", "subitem_source_identifier_type": "NCID"}]}, "item_6_subject_15": {"attribute_name": "NDC", "attribute_value_mlt": [{"subitem_subject": "440", "subitem_subject_scheme": "NDC"}]}, "item_6_text_30": {"attribute_name": "NIIタイプ", "attribute_value_mlt": [{"subitem_text_value": "Journal Article"}]}, "item_6_version_type_14": {"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": "Imai, Hiroshi", "creatorNameLang": "en"}, {"creatorName": "今井, 裕", "creatorNameLang": "ja"}], "nameIdentifiers": [{"nameIdentifier": "115028", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Chong, Sze Ning", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "115029", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "He, Jin-Hua", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "115030", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Nakashima, Jun-Ichi", "creatorNameLang": "en"}, {"creatorName": "中島, 淳一", "creatorNameLang": "ja"}], "nameIdentifiers": [{"nameIdentifier": "115031", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Hsia, Chih-Hao", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "115032", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Sakai, Takeshi", "creatorNameLang": "en"}, {"creatorName": "酒井, 剛", "creatorNameLang": "ja"}], "nameIdentifiers": [{"nameIdentifier": "115033", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Deguchi, Shuji", "creatorNameLang": "en"}, {"creatorName": "出口, 修至", "creatorNameLang": "ja"}], "nameIdentifiers": [{"nameIdentifier": "115034", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Koning, Nico", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "115035", "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": "2016-10-28"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "Extremely Strong 13CO J = 3→2 Line in the Water Fountain IRAS 16342-3814 Evidence for the Hot-Bottom Burning.pdf", "filesize": [{"value": "533.6 kB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_note", "mimetype": "application/pdf", "size": 533600.0, "url": {"label": "Extremely Strong 13CO J = 3→2 Line in the Water Fountain IRAS 16342-3814 Evidence for the Hot-Bottom Burning.pdf", "objectType": "fulltext", "url": "https://ir.kagoshima-u.ac.jp/record/9099/files/Extremely Strong 13CO J = 3→2 Line in the Water Fountain IRAS 16342-3814 Evidence for the Hot-Bottom Burning.pdf"}, "version_id": "bedd815d-b9ab-4325-bcaf-d337e62514af"}]}, "item_keyword": {"attribute_name": "キーワード", "attribute_value_mlt": [{"subitem_subject": "stars", "subitem_subject_language": "en", "subitem_subject_scheme": "Other"}, {"subitem_subject": "AGB and post-AGB -- stars", "subitem_subject_language": "en", "subitem_subject_scheme": "Other"}, {"subitem_subject": "individual (IRAS 16342-3814)", "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": "Extremely Strong 13CO J = 3→2 Line in the \"Water Fountain\" IRAS 16342-3814: Evidence for the Hot-Bottom Burning", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "Extremely Strong 13CO J = 3→2 Line in the \"Water Fountain\" IRAS 16342-3814: Evidence for the Hot-Bottom Burning", "subitem_title_language": "en"}]}, "item_type_id": "6", "owner": "18", "path": ["92"], "permalink_uri": "http://hdl.handle.net/10232/26221", "pubdate": {"attribute_name": "PubDate", "attribute_value": "2016-03-15"}, "publish_date": "2016-03-15", "publish_status": "0", "recid": "9099", "relation": {}, "relation_version_is_last": true, "title": ["Extremely Strong 13CO J = 3→2 Line in the \"Water Fountain\" IRAS 16342-3814: Evidence for the Hot-Bottom Burning"], "weko_shared_id": -1}
Extremely Strong 13CO J = 3→2 Line in the "Water Fountain" IRAS 16342-3814: Evidence for the Hot-Bottom Burning
http://hdl.handle.net/10232/26221
http://hdl.handle.net/10232/26221bf11fead-4e9d-42f6-b4f8-a6ad208eb090
名前 / ファイル | ライセンス | アクション |
---|---|---|
Extremely Strong 13CO J = 3→2 Line in the Water Fountain IRAS 16342-3814 Evidence for the Hot-Bottom Burning.pdf (533.6 kB)
|
|
Item type | 学術雑誌論文 / Journal Article(1) | |||||
---|---|---|---|---|---|---|
公開日 | 2016-03-15 | |||||
タイトル | ||||||
タイトル言語 | en | |||||
タイトル | Extremely Strong 13CO J = 3→2 Line in the "Water Fountain" IRAS 16342-3814: Evidence for the Hot-Bottom Burning | |||||
著者 |
今井, 裕
× 今井, 裕× Chong, Sze Ning× He, Jin-Hua× 中島, 淳一× Hsia, Chih-Hao× 酒井, 剛× 出口, 修至× Koning, Nico |
|||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
主題言語 | en | |||||
主題Scheme | Other | |||||
主題 | stars | |||||
キーワード | ||||||
主題言語 | en | |||||
主題Scheme | Other | |||||
主題 | AGB and post-AGB -- stars | |||||
キーワード | ||||||
主題言語 | en | |||||
主題Scheme | Other | |||||
主題 | individual (IRAS 16342-3814) | |||||
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 | |||||
要約(Abstract) | ||||||
内容記述タイプ | Other | |||||
内容記述 | We observed four "water fountain" sources in the CO J = 3→2 line emission with the Atacama Submillimeter Telescope Experiment (ASTE) 10m telescope in 2010–2011. The water fountain sources are evolved stars that form high-velocity collimated jets traced by H2O maser emission. The CO line was detected only from IRAS 16342-3814. The present work confirmed that the 12CO to 13CO line intensity ratio is ~1.5 at the systemic velocity. We discuss the origins of the very low 12CO-to-13CO intensity ratio, as possible evidence for "hot-bottom burning" in an oxygen-rich star, and the CO intensity variation in IRAS 16342-3814. | |||||
内容記述言語 | en | |||||
収録雑誌名 |
en : Publications of the Astronomical Society of Japan 巻 64, 号 5, p. 98, 発行日 2012 |
|||||
作成日 | ||||||
日付 | 2012-10-25 | |||||
日付タイプ | Issued | |||||
ISSN | ||||||
収録物識別子タイプ | PISSN | |||||
ISSN | 00046264 | |||||
NII書誌ID(雑誌) | ||||||
収録物識別子タイプ | NCID | |||||
NC ID | AA1082896X | |||||
DOI | ||||||
識別子タイプ | DOI | |||||
DOI | https://doi.org/10.1093/pasj/64.5.98 | |||||
権利 | ||||||
権利情報の言語 | en | |||||
権利情報 | Astronomical Society of Japan | |||||
出版タイプ | ||||||
出版タイプ | VoR | |||||
出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||
NDC | ||||||
主題Scheme | NDC | |||||
主題 | 440 | |||||
公開者・出版者 | ||||||
出版者言語 | en | |||||
出版者 | Astronomical Society of Japan | |||||
公開者・出版者 | ||||||
出版者言語 | ja | |||||
出版者 | 日本天文学会 |