ログイン
言語:

WEKO3

  • トップ
  • ランキング
To
lat lon distance
To

Field does not validate



インデックスリンク

インデックスツリー

メールアドレスを入力してください。

WEKO

One fine body…

WEKO

One fine body…

アイテム

{"_buckets": {"deposit": "68aa147a-4699-434c-93b4-69c4ce658211"}, "_deposit": {"id": "15871", "owners": [], "pid": {"revision_id": 0, "type": "depid", "value": "15871"}, "status": "published"}, "_oai": {"id": "oai:soar-ir.repo.nii.ac.jp:00015871", "sets": ["1545"]}, "author_link": ["45943", "45944", "45945", "45946", "45947"], "item_1628147817048": {"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_6_biblio_info_6": {"attribute_name": "書誌情報", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2010-06-01", "bibliographicIssueDateType": "Issued"}, "bibliographicIssueNumber": "2", "bibliographicPageEnd": "1507", "bibliographicPageStart": "1497", "bibliographicVolumeNumber": "715", "bibliographic_titles": [{"bibliographic_title": "The Astrophysical Journal"}]}]}, "item_6_description_20": {"attribute_name": "抄録", "attribute_value_mlt": [{"subitem_description": "Several neutral species (Mg I, Si I, Ca I, Fe I) have been detected in a weak Mg II absorption line system (W-r (2796) similar to 0.15 angstrom) at z similar to 0.45 along the sightline toward HE0001-2340. These observations require extreme physical conditions, as noted in D\u0027Odorico. We place further constraints on the properties of this system by running a wide grid of photoionization models, determining that the absorbing cloud that produces the neutral absorption is extremely dense (similar to 100-1000 cm(-3)), cold (\u003c100 K), and has significant molecular content (similar to 72%-94%). Structures of this size and temperature have been detected in Milky Way CO surveys and have been predicted in hydrodynamic simulations of turbulent gas. In order to explain the observed line profiles in all neutral and singly ionized chemical transitions, the lines must suffer from unresolved saturation and/or the absorber must partially cover the broad emission line region of the background quasar. In addition to this highly unusual cloud, three other ordinary weak Mg II clouds (within densities of similar to 0.005 cm(-3) and temperatures of similar to 10,000 K) lie within 500 km s(-1) along the same sightline. We suggest that the \"bare molecular cloud,\" which appears to reside outside of a galaxy disk, may have had in situ star formation and may evolve into an ordinary weak Mg II absorbing cloud.", "subitem_description_type": "Abstract"}]}, "item_6_description_31": {"attribute_name": "フォーマット:mimeタイプ", "attribute_value_mlt": [{"subitem_description": "application/pdf", "subitem_description_type": "Other"}]}, "item_6_description_5": {"attribute_name": "引用", "attribute_value_mlt": [{"subitem_description": "The Astrophysical Journal. 715(2):1497-1507 (2010)", "subitem_description_type": "Other"}]}, "item_6_link_3": {"attribute_name": "信州大学研究者総覧へのリンク", "attribute_value_mlt": [{"subitem_link_text": "Misawa, Toru", "subitem_link_url": "http://soar-rd.shinshu-u.ac.jp/profile/ja.ypchuUkV.html"}]}, "item_6_link_67": {"attribute_name": "WoS", "attribute_value_mlt": [{"subitem_link_text": "Web of Science", "subitem_link_url": "http://gateway.isiknowledge.com/gateway/Gateway.cgi?\u0026GWVersion=2\u0026SrcAuth=ShinshuUniv\u0026SrcApp=ShinshuUniv\u0026DestLinkType=FullRecord\u0026DestApp=WOS\u0026KeyUT=000277642100061"}]}, "item_6_publisher_4": {"attribute_name": "出版者", "attribute_value_mlt": [{"subitem_publisher": "IOP PUBLISHING LTD"}]}, "item_6_relation_48": {"attribute_name": "DOI", "attribute_value_mlt": [{"subitem_relation_name": [{"subitem_relation_name_text": "10.1088/0004-637X/715/2/1497"}], "subitem_relation_type_id": {"subitem_relation_type_id_text": "https://doi.org/10.1088/0004-637X/715/2/1497", "subitem_relation_type_select": "DOI"}}]}, "item_6_rights_62": {"attribute_name": "権利", "attribute_value_mlt": [{"subitem_rights": "Copyright (c) 2010 The American Astronomical Society"}]}, "item_6_select_64": {"attribute_name": "著者版フラグ", "attribute_value_mlt": [{"subitem_select_item": "publisher"}]}, "item_6_source_id_35": {"attribute_name": "ISSN", "attribute_value_mlt": [{"subitem_source_identifier": "0004-637X", "subitem_source_identifier_type": "ISSN"}]}, "item_6_source_id_39": {"attribute_name": "NII ISSN", "attribute_value_mlt": [{"subitem_source_identifier": "0004-637X", "subitem_source_identifier_type": "ISSN"}]}, "item_6_source_id_40": {"attribute_name": "書誌レコードID", "attribute_value_mlt": [{"subitem_source_identifier": "AA00553253", "subitem_source_identifier_type": "NCID"}]}, "item_6_text_69": {"attribute_name": "wosonly authkey", "attribute_value_mlt": [{"subitem_text_value": "galaxies: evolution; galaxies: halos; intergalactic medium; quasars: absorption lines"}]}, "item_6_text_70": {"attribute_name": "wosonly keywords", "attribute_value_mlt": [{"subitem_text_value": "WEAK MGII ABSORBERS; ABSORPTION-SELECTED GALAXIES; LY-ALPHA ABSORPTION; II ABSORBERS; DARK-MATTER; COLD GAS; GALACTIC WINDS; HALO GAS; HYDROGEN; SYSTEMS"}]}, "item_6_textarea_68": {"attribute_name": "wosonly abstract", "attribute_value_mlt": [{"subitem_textarea_value": "Several neutral species (Mg I, Si I, Ca I, Fe I) have been detected in a weak Mg II absorption line system (W-r (2796) similar to 0.15 angstrom) at z similar to 0.45 along the sightline toward HE0001-2340. These observations require extreme physical conditions, as noted in D\u0027Odorico. We place further constraints on the properties of this system by running a wide grid of photoionization models, determining that the absorbing cloud that produces the neutral absorption is extremely dense (similar to 100-1000 cm(-3)), cold (\u003c100 K), and has significant molecular content (similar to 72%-94%). Structures of this size and temperature have been detected in Milky Way CO surveys and have been predicted in hydrodynamic simulations of turbulent gas. In order to explain the observed line profiles in all neutral and singly ionized chemical transitions, the lines must suffer from unresolved saturation and/or the absorber must partially cover the broad emission line region of the background quasar. In addition to this highly unusual cloud, three other ordinary weak Mg II clouds (within densities of similar to 0.005 cm(-3) and temperatures of similar to 10,000 K) lie within 500 km s(-1) along the same sightline. We suggest that the \"bare molecular cloud,\" which appears to reside outside of a galaxy disk, may have had in situ star formation and may evolve into an ordinary weak Mg II absorbing cloud."}]}, "item_creator": {"attribute_name": "著者", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "Jones,  Therese M."}], "nameIdentifiers": [{"nameIdentifier": "45943", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Misawa,  Toru"}], "nameIdentifiers": [{"nameIdentifier": "45944", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Charlton,  Jane C."}], "nameIdentifiers": [{"nameIdentifier": "45945", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Mshar,  Andrew C."}], "nameIdentifiers": [{"nameIdentifier": "45946", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Ferland,  Gary J."}], "nameIdentifiers": [{"nameIdentifier": "45947", "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": "2015-09-28"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "BARE_MOLECULAR_CLOUD.pdf", "filesize": [{"value": "421.3 kB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_note", "mimetype": "application/pdf", "size": 421300.0, "url": {"label": "BARE_MOLECULAR_CLOUD.pdf", "url": "https://soar-ir.repo.nii.ac.jp/record/15871/files/BARE_MOLECULAR_CLOUD.pdf"}, "version_id": "546cd6ad-323d-420d-90d0-b81c015759cb"}]}, "item_keyword": {"attribute_name": "キーワード", "attribute_value_mlt": [{"subitem_subject": "galaxies: evolution", "subitem_subject_scheme": "Other"}, {"subitem_subject": "galaxies: halos", "subitem_subject_scheme": "Other"}, {"subitem_subject": "intergalactic medium", "subitem_subject_scheme": "Other"}, {"subitem_subject": "quasars: absorption lines", "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": "A BARE MOLECULAR CLOUD AT z similar to 0.45", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "A BARE MOLECULAR CLOUD AT z similar to 0.45", "subitem_title_language": "en"}]}, "item_type_id": "6", "owner": "1", "path": ["1545"], "permalink_uri": "http://hdl.handle.net/10091/10712", "pubdate": {"attribute_name": "PubDate", "attribute_value": "2010-10-18"}, "publish_date": "2010-10-18", "publish_status": "0", "recid": "15871", "relation": {}, "relation_version_is_last": true, "title": ["A BARE MOLECULAR CLOUD AT z similar to 0.45"], "weko_shared_id": -1}
  1. 100 全学教育センター
  2. 1001 学術論文

A BARE MOLECULAR CLOUD AT z similar to 0.45

http://hdl.handle.net/10091/10712
http://hdl.handle.net/10091/10712
e41ad45f-89d8-4263-b285-8bdd319f4689
名前 / ファイル ライセンス アクション
BARE_MOLECULAR_CLOUD.pdf BARE_MOLECULAR_CLOUD.pdf (421.3 kB)
Item type 学術雑誌論文 / Journal Article(1)
公開日 2010-10-18
タイトル
言語 en
タイトル A BARE MOLECULAR CLOUD AT z similar to 0.45
言語
言語 eng
キーワード
主題Scheme Other
主題 galaxies: evolution
キーワード
主題Scheme Other
主題 galaxies: halos
キーワード
主題Scheme Other
主題 intergalactic medium
キーワード
主題Scheme Other
主題 quasars: absorption lines
資源タイプ
資源 http://purl.org/coar/resource_type/c_6501
タイプ journal article
著者 Jones, Therese M.

× Jones, Therese M.

WEKO 45943

Jones, Therese M.

Search repository
Misawa, Toru

× Misawa, Toru

WEKO 45944

Misawa, Toru

Search repository
Charlton, Jane C.

× Charlton, Jane C.

WEKO 45945

Charlton, Jane C.

Search repository
Mshar, Andrew C.

× Mshar, Andrew C.

WEKO 45946

Mshar, Andrew C.

Search repository
Ferland, Gary J.

× Ferland, Gary J.

WEKO 45947

Ferland, Gary J.

Search repository
信州大学研究者総覧へのリンク
氏名 Misawa, Toru
URL http://soar-rd.shinshu-u.ac.jp/profile/ja.ypchuUkV.html
出版者
出版者 IOP PUBLISHING LTD
引用
内容記述タイプ Other
内容記述 The Astrophysical Journal. 715(2):1497-1507 (2010)
書誌情報 The Astrophysical Journal

巻 715, 号 2, p. 1497-1507, 発行日 2010-06-01
抄録
内容記述タイプ Abstract
内容記述 Several neutral species (Mg I, Si I, Ca I, Fe I) have been detected in a weak Mg II absorption line system (W-r (2796) similar to 0.15 angstrom) at z similar to 0.45 along the sightline toward HE0001-2340. These observations require extreme physical conditions, as noted in D'Odorico. We place further constraints on the properties of this system by running a wide grid of photoionization models, determining that the absorbing cloud that produces the neutral absorption is extremely dense (similar to 100-1000 cm(-3)), cold (<100 K), and has significant molecular content (similar to 72%-94%). Structures of this size and temperature have been detected in Milky Way CO surveys and have been predicted in hydrodynamic simulations of turbulent gas. In order to explain the observed line profiles in all neutral and singly ionized chemical transitions, the lines must suffer from unresolved saturation and/or the absorber must partially cover the broad emission line region of the background quasar. In addition to this highly unusual cloud, three other ordinary weak Mg II clouds (within densities of similar to 0.005 cm(-3) and temperatures of similar to 10,000 K) lie within 500 km s(-1) along the same sightline. We suggest that the "bare molecular cloud," which appears to reside outside of a galaxy disk, may have had in situ star formation and may evolve into an ordinary weak Mg II absorbing cloud.
ISSN
収録物識別子タイプ ISSN
収録物識別子 0004-637X
書誌レコードID
収録物識別子タイプ NCID
収録物識別子 AA00553253
DOI
識別子タイプ DOI
関連識別子 https://doi.org/10.1088/0004-637X/715/2/1497
関連名称 10.1088/0004-637X/715/2/1497
権利
権利情報 Copyright (c) 2010 The American Astronomical Society
出版タイプ
出版タイプ VoR
出版タイプResource http://purl.org/coar/version/c_970fb48d4fbd8a85
WoS
表示名 Web of Science
URL http://gateway.isiknowledge.com/gateway/Gateway.cgi?&GWVersion=2&SrcAuth=ShinshuUniv&SrcApp=ShinshuUniv&DestLinkType=FullRecord&DestApp=WOS&KeyUT=000277642100061
戻る
0
views
See details
Views

Versions

Ver.1 2021-03-01 10:11:46.491554
Show All versions

Share

Mendeley Twitter Facebook Print Addthis

Cite as

エクスポート

OAI-PMH
  • OAI-PMH JPCOAR
  • OAI-PMH DublinCore
  • OAI-PMH DDI
Other Formats
  • JSON
  • BIBTEX

Confirm


Powered by WEKO3


Powered by WEKO3