{"_buckets": {"deposit": "06c1bf04-636c-45c0-8ff6-48adabb5cbcb"}, "_deposit": {"created_by": 17, "id": "2002688", "owner": "17", "owners": [17], "owners_ext": {"displayname": "repository", "username": "repository"}, "pid": {"revision_id": 0, "type": "depid", "value": "2002688"}, "status": "published"}, "_oai": {"id": "oai:nagoya.repo.nii.ac.jp:02002688"}, "author_link": [], "item_1615768549627": {"attribute_name": "\u51fa\u7248\u30bf\u30a4\u30d7", "attribute_value_mlt": [{"subitem_version_resource": "http://purl.org/coar/version/c_ab4af688f83e57aa", "subitem_version_type": "AM"}]}, "item_1629683748249": {"attribute_name": "\u65e5\u4ed8", "attribute_value_mlt": [{"subitem_date_issued_datetime": "2022-08-01", "subitem_date_issued_type": "Available"}]}, "item_9_biblio_info_6": {"attribute_name": "\u66f8\u8a8c\u60c5\u5831", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2021-08", "bibliographicIssueDateType": "Issued"}, "bibliographicIssueNumber": "4", "bibliographicPageEnd": "879", "bibliographicPageStart": "864", "bibliographicVolumeNumber": "73", "bibliographic_titles": [{"bibliographic_title": "Publications of the Astronomical Society of Japan", "bibliographic_titleLang": "en"}]}]}, "item_9_description_4": {"attribute_name": "\u5185\u5bb9\u8a18\u8ff0", "attribute_value_mlt": [{"subitem_description": "We present a new method to evaluate the dust extinction (AV) along the line of sight using the InfraRed Survey Facility (IRSF) near-infrared (NIR) data of the Large Magellanic Cloud (LMC) H\u2009i ridge region. In our method, we estimate an AV value for each star from the NIR color excess and sort them from bluer to redder in each line of sight. Using the percentile values of the sorted AV, we construct a new three-dimensional AV map. We compare the resultant AV map with the total hydrogen column density N(H) traced by velocity-resolved H\u2009i and CO observations. In the LMC H\u2009i ridge region, Fukui et al. (2017, PASJ, 69, L5) found two velocity components and an intermediate velocity one bridging them. Comparing our three-dimensional AV maps with N(H) maps at the different velocities, we find that the dust geometry is consistent with the scenario of ongoing gas collision between the two velocities as suggested in the previous study. In addition, we find a difference by a factor of 2 in AV/N(H) between the two velocity components, which suggests that inflow gas from the Small Magellanic Clouds (SMC) is mixed in this region. Overall, our results support triggered star formation in 30 Doradus due to the large-scale gas collision caused by tidal interaction between the LMC and the SMC.", "subitem_description_language": "en", "subitem_description_type": "Abstract"}]}, "item_9_publisher_32": {"attribute_name": "\u51fa\u7248\u8005", "attribute_value_mlt": [{"subitem_publisher": "Oxford University Press", "subitem_publisher_language": "en"}]}, "item_9_relation_43": {"attribute_name": "\u95a2\u9023\u60c5\u5831", "attribute_value_mlt": [{"subitem_relation_type": "isVersionOf", "subitem_relation_type_id": {"subitem_relation_type_id_text": "https://doi.org/10.1093/pasj/psab052", "subitem_relation_type_select": "DOI"}}]}, "item_9_rights_12": {"attribute_name": "\u6a29\u5229", "attribute_value_mlt": [{"subitem_rights": "This is a pre-copyedited, author-produced version of an article accepted for publication in [Publications of the Astronomical Society of Japan] following peer review. The version of record [Takuya Furuta, Hidehiro Kaneda, Takuma Kokusho, Yasushi Nakajima, Yasuo Fukui, Kisetsu Tsuge, Three-dimensional dust geometry of the LMC H\u2009i ridge region as revealed by the IRSF/SIRIUS survey, Publications of the Astronomical Society of Japan, Volume 73, Issue 4, August 2021, Pages 864\u2013879, https://doi.org/10.1093/pasj/psab052] is available online at: https://doi.org/10.1093/pasj/psab052.", "subitem_rights_language": "en"}]}, "item_9_source_id_7": {"attribute_name": "\u53ce\u9332\u7269\u8b58\u5225\u5b50", "attribute_value_mlt": [{"subitem_source_identifier": "0004-6264", "subitem_source_identifier_type": "PISSN"}]}, "item_access_right": {"attribute_name": "\u30a2\u30af\u30bb\u30b9\u6a29", "attribute_value_mlt": [{"subitem_access_right": "embargoed access", "subitem_access_right_uri": "http://purl.org/coar/access_right/c_f1cf"}]}, "item_creator": {"attribute_name": "\u8457\u8005", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "Furuta, Takuya", "creatorNameLang": "en"}]}, {"creatorNames": [{"creatorName": "Kaneda, Hidehiro", "creatorNameLang": "en"}]}, {"creatorNames": [{"creatorName": "Kokusho, Takuma", "creatorNameLang": "en"}]}, {"creatorNames": [{"creatorName": "Nakajima, Yasushi", "creatorNameLang": "en"}]}, {"creatorNames": [{"creatorName": "Fukui, Yasuo", "creatorNameLang": "en"}]}, {"creatorNames": [{"creatorName": "Tsuge, Kisetsu", "creatorNameLang": "en"}]}]}, "item_files": {"attribute_name": "\u30d5\u30a1\u30a4\u30eb\u60c5\u5831", "attribute_type": "file", "attribute_value_mlt": [{"accessrole": "open_date", "date": [{"dateType": "Available", "dateValue": "2022-08-01"}], "displaytype": "detail", "download_preview_message": "Download / Preview is available from 2022/7/31.", "file_order": 0, "filename": "2105_05421.pdf", "filesize": [{"value": "1.7 MB"}], "format": "application/pdf", "future_date_message": "Download is available from 2022/7/31.", "is_thumbnail": false, "mimetype": "application/pdf", "size": 1700000.0, "url": {"objectType": "fulltext", "url": "https://nagoya.repo.nii.ac.jp/record/2002688/files/2105_05421.pdf"}, "version_id": "df49629c-a99a-49c4-bcaf-1d93b0b8a91b"}]}, "item_keyword": {"attribute_name": "\u30ad\u30fc\u30ef\u30fc\u30c9", "attribute_value_mlt": [{"subitem_subject": "(galaxies:) Magellanic Clouds", "subitem_subject_scheme": "Other"}, {"subitem_subject": "infrared: ISM", "subitem_subject_scheme": "Other"}, {"subitem_subject": "(ISM:) dust", "subitem_subject_scheme": "Other"}, {"subitem_subject": "extinction", "subitem_subject_scheme": "Other"}, {"subitem_subject": "ISM: structure", "subitem_subject_scheme": "Other"}]}, "item_language": {"attribute_name": "\u8a00\u8a9e", "attribute_value_mlt": [{"subitem_language": "eng"}]}, "item_resource_type": {"attribute_name": "\u8cc7\u6e90\u30bf\u30a4\u30d7", "attribute_value_mlt": [{"resourcetype": "journal article", "resourceuri": "http://purl.org/coar/resource_type/c_6501"}]}, "item_title": "Three-dimensional dust geometry of the LMC H\u2009i ridge region as revealed by the IRSF/SIRIUS survey", "item_titles": {"attribute_name": "\u30bf\u30a4\u30c8\u30eb", "attribute_value_mlt": [{"subitem_title": "Three-dimensional dust geometry of the LMC H\u2009i ridge region as revealed by the IRSF/SIRIUS survey", "subitem_title_language": "en"}]}, "item_type_id": "40001", "owner": "17", "path": ["336/695/696"], "permalink_uri": "http://hdl.handle.net/2237/0002002688", "pubdate": {"attribute_name": "PubDate", "attribute_value": "2022-05-09"}, "publish_date": "2022-05-09", "publish_status": "0", "recid": "2002688", "relation": {}, "relation_version_is_last": true, "title": ["Three-dimensional dust geometry of the LMC H\u2009i ridge region as revealed by the IRSF/SIRIUS survey"], "weko_shared_id": -1}