{"_buckets": {"deposit": "271f498a-da44-4e98-befb-8fef8ff62a2a"}, "_deposit": {"created_by": 3, "id": "13283", "owners": [3], "pid": {"revision_id": 0, "type": "depid", "value": "13283"}, "status": "published"}, "_oai": {"id": "oai:ir.kagoshima-u.ac.jp:00013283", "sets": ["92"]}, "author_link": ["116470", "116465", "116461", "116464", "116468", "116466", "116467", "116462", "116463", "116469"], "item_6_biblio_info_5": {"attribute_name": "収録雑誌名", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2009", "bibliographicIssueDateType": "Issued"}, "bibliographicIssueNumber": "6", "bibliographicPageEnd": "1372", "bibliographicPageStart": "1365", "bibliographicVolumeNumber": "61", "bibliographic_titles": [{"bibliographic_title": "Publications of the Astronomical Society of Japan"}]}]}, "item_6_date_6": {"attribute_name": "作成日", "attribute_value_mlt": [{"subitem_date_issued_datetime": "2009-12-25"}]}, "item_6_description_4": {"attribute_name": "要約(Abstract)", "attribute_value_mlt": [{"subitem_description": "We observed CO J = 3–2 emission from \"water-fountain\" sources, which exhibit high-velocity collimated stellar jets traced by H2O maser emission, with the Atacama Submillimeter Telescope Experiment (ASTE) 10m telescope. We detected CO emission from two sources: IRAS 16342-3814 and IRAS 18286-0959. The IRAS 16342-3814 CO emission exhibits a spectrum that could be well fit to a Gaussian profile, rather than to a parabolic profile, with a velocity width (FWHM) of 158±6 km s^-1 and an intensity peak at V_LSR= 50±2 km s^-1. The mass-loss rate of the star is estimated to be ~2.9×10^-5 M yr^-1. Our morpho-kinematic models suggest that the CO emission is optically thin, and associated with a bipolar outflow rather than with a (cold and relatively small) torus. The IRAS 18286-0959 CO emission has a velocity width (FWHM) of 3.0±0.2 km s ^-1, smaller than typically seen in AGB envelopes. The narrow velocity width of the CO emission suggests that it originates from either an interstellar molecular cloud or a slowly-rotating circumstellar envelope that harbors the H2O maser source.", "subitem_description_type": "Other"}]}, "item_6_full_name_3": {"attribute_name": "別言語の著者", "attribute_value_mlt": [{"nameIdentifiers": [{"nameIdentifier": "116467", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "今井, 裕"}]}, {"nameIdentifiers": [{"nameIdentifier": "116468", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "中島, 淳一"}]}, {"nameIdentifiers": [{"nameIdentifier": "116469", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "浮田, 信治"}]}, {"nameIdentifiers": [{"nameIdentifier": "116470", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "出口, 修至"}]}]}, "item_6_publisher_23": {"attribute_name": "公開者・出版者", "attribute_value_mlt": [{"subitem_publisher": "Astronomical Society of Japan"}]}, "item_6_relation_11": {"attribute_name": "DOI", "attribute_value_mlt": 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[{"creatorName": "KONING, Nico"}], "nameIdentifiers": [{"nameIdentifier": "116466", "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": "2016-10-31"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "CO J = 3-2 Emission from the Water Fountain Sources IRAS 16342-3814 and IRAS 18286-0959.pdf", "filesize": [{"value": "1.3 MB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_free", "mimetype": "application/pdf", "size": 1300000.0, "url": {"label": "CO J = 3-2 Emission from the Water Fountain Sources IRAS 16342-3814 and IRAS 18286-0959.pdf", "url": "https://ir.kagoshima-u.ac.jp/record/13283/files/CO J = 3-2 Emission from the Water Fountain Sources IRAS 16342-3814 and IRAS 18286-0959.pdf"}, "version_id": 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"http://hdl.handle.net/10232/26220", "pubdate": {"attribute_name": "公開日", "attribute_value": "2016-03-15"}, "publish_date": "2016-03-15", "publish_status": "0", "recid": "13283", "relation": {}, "relation_version_is_last": true, "title": ["CO J = 3–2 Emission from the \"Water Fountain\" Sources IRAS 16342-3814 and IRAS 18286-0959"], "weko_shared_id": 3}