{"_buckets": {"deposit": "353d43c0-a104-403e-a5fd-09130a817a63"}, "_deposit": {"id": "28839", "owners": [], "pid": {"revision_id": 0, "type": "depid", "value": "28839"}, "status": "published"}, "_oai": {"id": "oai:nagoya.repo.nii.ac.jp:00028839", "sets": ["696"]}, "author_link": ["94913", "94914"], "item_10_biblio_info_6": {"attribute_name": "書誌情報", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2019-09", "bibliographicIssueDateType": "Issued"}, "bibliographicIssueNumber": "2", "bibliographicPageEnd": "2649", "bibliographicPageStart": "2644", "bibliographicVolumeNumber": "488", "bibliographic_titles": [{"bibliographic_title": "Monthly Notices of the Royal Astronomical Society", "bibliographic_titleLang": "en"}]}]}, "item_10_description_4": {"attribute_name": "抄録", "attribute_value_mlt": [{"subitem_description": "We perform radiation hydrodynamical simulations in spherical symmetry in order to investigate the formation of very low mass objects, i.e. brown dwarfs, by external compression. According to the Jeans stability criterion, a very low mass molecular cloud core must reach a very high density in order to become gravitationally unstable. One possibility to create such a high density is the compression by turbulent flows within the larger molecular cloud. Using our self-developed radiation hydrodynamics code, we aim to test the validity of this scenario, and to constrain the strength of the turbulence that is needed. We find that the probability for sufficiently strong and long-lived turbulence is very low under typical conditions even when using very optimistic assumptions, and therefore conclude that turbulent compression is unlikely to be the dominant mechanism for creating brown dwarfs. We also investigate the properties of objects formed by this turbulent compression process. Specifically, we compare the lifetime of the first core stage for the cases with and without external compression. We confirm our previous findings that the first core lifetime increases by about an order of magnitude at the extremely low-mass end, but this increase is somewhat less dramatic and occurs at even lower masses than in our previous work, in which no external compression was present.", "subitem_description_language": "en", "subitem_description_type": "Abstract"}]}, "item_10_publisher_32": {"attribute_name": "出版者", "attribute_value_mlt": [{"subitem_publisher": "Oxford University Press", "subitem_publisher_language": "en"}]}, "item_10_relation_11": {"attribute_name": "DOI", "attribute_value_mlt": [{"subitem_relation_type": "isVersionOf", "subitem_relation_type_id": {"subitem_relation_type_id_text": "https://doi.org/10.1093/mnras/stz1892", "subitem_relation_type_select": "DOI"}}]}, "item_10_rights_12": {"attribute_name": "権利", "attribute_value_mlt": [{"subitem_rights": "This article has been accepted for publication in [Monthly Notices of the Royal Astronomical Society] ©: [2019] [authors] Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.", "subitem_rights_language": "en"}]}, "item_10_select_15": {"attribute_name": "著者版フラグ", "attribute_value_mlt": [{"subitem_select_item": "publisher"}]}, "item_10_source_id_61": {"attribute_name": "ISSN（print）", "attribute_value_mlt": [{"subitem_source_identifier": "0035-8711", "subitem_source_identifier_type": "PISSN"}]}, "item_1615787544753": {"attribute_name": "出版タイプ", "attribute_value_mlt": [{"subitem_version_resource": "http://purl.org/coar/version/c_970fb48d4fbd8a85", "subitem_version_type": "VoR"}]}, "item_access_right": {"attribute_name": "アクセス権", "attribute_value_mlt": [{"subitem_access_right": "open access", "subitem_access_right_uri": "http://purl.org/coar/access_right/c_abf2"}]}, "item_creator": {"attribute_name": "著者", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "Stamer, Torsten", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "94913", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Inutsuka, Shu-ichiro", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "94914", "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": "2019-12-20"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "stz1892.pdf", "filesize": [{"value": "318.4 kB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_note", "mimetype": "application/pdf", "size": 318400.0, "url": {"label": "stz1892", "objectType": "fulltext", "url": "https://nagoya.repo.nii.ac.jp/record/28839/files/stz1892.pdf"}, "version_id": "9f0b9a4d-671a-4d12-a5e4-12e495ebe6f3"}]}, "item_keyword": {"attribute_name": "キーワード", "attribute_value_mlt": [{"subitem_subject": "brown dwarfs", "subitem_subject_scheme": "Other"}, {"subitem_subject": "stars: formation", "subitem_subject_scheme": "Other"}, {"subitem_subject": "stars: pre-main-sequence", "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": "Constraints on the formation of brown dwarfs by turbulent compression", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "Constraints on the formation of brown dwarfs by turbulent compression", "subitem_title_language": "en"}]}, "item_type_id": "10", "owner": "1", "path": ["696"], "permalink_uri": "http://hdl.handle.net/2237/00031026", "pubdate": {"attribute_name": "PubDate", "attribute_value": "2019-12-20"}, "publish_date": "2019-12-20", "publish_status": "0", "recid": "28839", "relation": {}, "relation_version_is_last": true, "title": ["Constraints on the formation of brown dwarfs by turbulent compression"], "weko_shared_id": -1}