{"_buckets": {"deposit": "25f375df-78b6-44c2-89a5-955151a08898"}, "_deposit": {"created_by": 3, "id": "6098", "owners": [3], "pid": {"revision_id": 0, "type": "depid", "value": "6098"}, "status": "published"}, "_oai": {"id": "oai:ir.kagoshima-u.ac.jp:00006098", "sets": ["92"]}, "author_link": ["123356", "123359", "123361", "123358", "123363", "123365", "123360", "123357", "123362", "123364", "123355", "123354"], "item_6_biblio_info_5": {"attribute_name": "収録雑誌名", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2010", "bibliographicIssueDateType": "Issued"}, "bibliographicIssueNumber": "1", "bibliographicPageEnd": "277", "bibliographicPageStart": "267", "bibliographicVolumeNumber": "721", "bibliographic_titles": [{"bibliographic_title": "The Astronomical Journal"}]}]}, "item_6_date_6": {"attribute_name": "作成日", "attribute_value_mlt": [{"subitem_date_issued_datetime": "2010-09-20"}]}, "item_6_description_4": {"attribute_name": "要約(Abstract)", "attribute_value_mlt": [{"subitem_description": "We have conducted Very Long Baseline Array phase-referencing monitoring of H2O masers around the red supergiant, S Persei, for six years.We have fitted maser motions to a simple expanding-shell model with a common annual parallax and stellar proper motion, and obtained the annual parallax as 0.413 ± 0.017 mas and the stellar proper motion as (-0.49 ± 0.23 mas yr^-1, -1.19 ± 0.20 mas yr^-1) in right ascension and declination, respectively. The obtained annual parallax corresponds to the trigonometric distance of 2.42[+0.11 -0.09] kpc. Assuming a Galactocentric distance of the Sun of 8.5 kpc, the circular rotational velocity of the local standard of rest at a distance of the Sun of 220 km s^-1, and a flat Galactic rotation curve, S Persei is suggested to have a non-circular motion deviating from the Galactic circular rotation for 15 km s^-1, which is mainly dominated by the anti-rotation direction component of 12.9 ± 2.9 km s^-1. This red supergiant is thought to belong to the OB association, Per OB1, so that this non-circular motion is representative of a motion of the OB association in the MilkyWay. This non-circular motion is somewhat larger than that explained by the standard density-wave theory for a spiral galaxy and is attributed to either a cluster shuffling of the OB association, or to non-linear interactions between non-stationary spiral arms and multi-phase interstellar media. The latter comes from a new view of a spiral arm formation in the Milky Way suggested by recent large N-body/smoothed particle hydrodynamics numerical simulations.", "subitem_description_type": "Other"}]}, "item_6_full_name_3": {"attribute_name": "別言語の著者", "attribute_value_mlt": [{"nameIdentifiers": [{"nameIdentifier": "123360", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "朝木, 義晴"}]}, {"nameIdentifiers": [{"nameIdentifier": "123361", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "出口, 修至"}]}, {"nameIdentifiers": [{"nameIdentifier": "123362", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "今井, 裕"}]}, {"nameIdentifiers": [{"nameIdentifier": "123363", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "蜂須賀, 一也"}]}, {"nameIdentifiers": [{"nameIdentifier": "123364", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "三好, 真"}]}, {"nameIdentifiers": [{"nameIdentifier": "123365", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "本間, 希樹"}]}]}, "item_6_publisher_23": {"attribute_name": "公開者・出版者", "attribute_value_mlt": [{"subitem_publisher": "American Astronomical Society"}, {"subitem_publisher": "IOP Publishing"}]}, "item_6_relation_11": {"attribute_name": "DOI", "attribute_value_mlt": [{"subitem_relation_type": "isIdenticalTo", "subitem_relation_type_id": {"subitem_relation_type_id_text": "info:doi/10.1088/0004-637X/721/1/267", "subitem_relation_type_select": "DOI"}}]}, "item_6_rights_12": {"attribute_name": "権利", "attribute_value_mlt": [{"subitem_rights": "American Astronomical Society"}]}, "item_6_source_id_7": {"attribute_name": "ISSN", "attribute_value_mlt": [{"subitem_source_identifier": "0004-6256", "subitem_source_identifier_type": "ISSN"}]}, "item_6_source_id_9": {"attribute_name": "NII書誌ID", "attribute_value_mlt": [{"subitem_source_identifier": "AA00552749", "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": "ASAKI, Yoshiharu"}], "nameIdentifiers": [{"nameIdentifier": "123354", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "DEGUCHI, Shuji"}], "nameIdentifiers": [{"nameIdentifier": "123355", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "IMAI, Hiroshi"}], "nameIdentifiers": [{"nameIdentifier": "123356", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "HACHISUKA, Kazuya"}], "nameIdentifiers": [{"nameIdentifier": "123357", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "MIYOSHI, Makoto"}], "nameIdentifiers": [{"nameIdentifier": "123358", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "HONMA, Mareki"}], "nameIdentifiers": [{"nameIdentifier": "123359", "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": "1.pdf", "filesize": [{"value": "1.5 MB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_free", "mimetype": "application/pdf", "size": 1500000.0, "url": {"label": "1.pdf", "url": "https://ir.kagoshima-u.ac.jp/record/6098/files/1.pdf"}, "version_id": "5e008683-164e-4734-8f34-a161b2414cd5"}]}, "item_keyword": {"attribute_name": "キーワード", "attribute_value_mlt": [{"subitem_subject": "Galaxy: structure -- masers -- supergiants", "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": "DISTANCE AND PROPER MOTION MEASUREMENT OF THE RED SUPERGIANT, S PERSEI, WITH VLBI H2O MASER ASTROMETRY", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "DISTANCE AND PROPER MOTION MEASUREMENT OF THE RED SUPERGIANT, S PERSEI, WITH VLBI H2O MASER ASTROMETRY"}]}, "item_type_id": "6", "owner": "3", "path": ["92"], "permalink_uri": "http://hdl.handle.net/10232/26181", "pubdate": {"attribute_name": "公開日", "attribute_value": "2016-03-15"}, "publish_date": "2016-03-15", "publish_status": "0", "recid": "6098", "relation": {}, "relation_version_is_last": true, "title": ["DISTANCE AND PROPER MOTION MEASUREMENT OF THE RED SUPERGIANT, S PERSEI, WITH VLBI H2O MASER ASTROMETRY"], "weko_shared_id": 3}