{"created":"2023-07-25T08:07:06.437269+00:00","id":6098,"links":{},"metadata":{"_buckets":{"deposit":"25f375df-78b6-44c2-89a5-955151a08898"},"_deposit":{"created_by":18,"id":"6098","owners":[18],"pid":{"revision_id":0,"type":"depid","value":"6098"},"status":"published"},"_oai":{"id":"oai:ir.kagoshima-u.ac.jp:00006098","sets":["54:92"]},"author_link":["123354","123355","123356","123357","123358","123359"],"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","bibliographic_titleLang":"en"}]}]},"item_6_date_6":{"attribute_name":"作成日","attribute_value_mlt":[{"subitem_date_issued_datetime":"2010-09-20","subitem_date_issued_type":"Issued"}]},"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_language":"en","subitem_description_type":"Other"}]},"item_6_publisher_23":{"attribute_name":"公開者・出版者","attribute_value_mlt":[{"subitem_publisher":"American Astronomical Society/IOP Publishing","subitem_publisher_language":"en"}]},"item_6_relation_11":{"attribute_name":"DOI","attribute_value_mlt":[{"subitem_relation_type_id":{"subitem_relation_type_id_text":"https://doi.org/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","subitem_rights_language":"en"}]},"item_6_source_id_7":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"00046256","subitem_source_identifier_type":"PISSN"}]},"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_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","creatorNameLang":"en"},{"creatorName":"朝木, 義晴","creatorNameLang":"ja"}],"nameIdentifiers":[{"nameIdentifier":"123354","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Deguchi, Shuji","creatorNameLang":"en"},{"creatorName":"出口, 修至","creatorNameLang":"ja"}],"nameIdentifiers":[{"nameIdentifier":"123355","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Imai, Hiroshi","creatorNameLang":"en"},{"creatorName":"今井, 裕","creatorNameLang":"ja"}],"nameIdentifiers":[{"nameIdentifier":"123356","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Hachisuka, Kazuya","creatorNameLang":"en"},{"creatorName":"蜂須賀, 一也","creatorNameLang":"ja"}],"nameIdentifiers":[{"nameIdentifier":"123357","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Miyoshi, Makoto","creatorNameLang":"en"},{"creatorName":"三好, 真","creatorNameLang":"ja"}],"nameIdentifiers":[{"nameIdentifier":"123358","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Honma, Mareki","creatorNameLang":"en"},{"creatorName":"本間, 希樹","creatorNameLang":"ja"}],"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","filename":"1.pdf","filesize":[{"value":"1.5 MB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"1.pdf","objectType":"fulltext","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_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":"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","subitem_title_language":"en"}]},"item_type_id":"6","owner":"18","path":["92"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2016-03-15"},"publish_date":"2016-03-15","publish_status":"0","recid":"6098","relation_version_is_last":true,"title":["DISTANCE AND PROPER MOTION MEASUREMENT OF THE RED SUPERGIANT, S PERSEI, WITH VLBI H2O MASER ASTROMETRY"],"weko_creator_id":"18","weko_shared_id":-1},"updated":"2024-02-07T07:13:17.169022+00:00"}