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J-GLOBAL ID：202202228909672631   整理番号：22A0742265

ODYSSEUS調査 動機付けと最初の結果:CVSO109の降着,放出,および円盤照射【JST・京大機械翻訳】

The ODYSSEUS Survey. Motivation and First Results: Accretion, Ejection, and Disk Irradiation of CVSO 109

著者 (72件)： Espaillat C. C. (Institute for Astrophysical Research, Department of Astronomy, Boston University, 725 Commonwealth Avenue, Boston, MA 02215, USA) ,  Herczeg G. J. (Kavli Institute for Astronomy and Astrophysics, Peking University, Yiheyuan 5, Haidian Qu, 100871 Beijing, People’s Republic of China) ,  Herczeg G. J. (Department of Astronomy, Peking University, Yiheyuan 5, Haidian Qu, 100871 Beijing, People’s Republic of China) ,  Thanathibodee T. (Department of Astronomy, University of Michigan, 1085 South University Avenue, Ann Arbor, MI 48109, USA) ,  Pittman C. (Institute for Astrophysical Research, Department of Astronomy, Boston University, 725 Commonwealth Avenue, Boston, MA 02215, USA) ,  Calvet N. (Department of Astronomy, University of Michigan, 1085 South University Avenue, Ann Arbor, MI 48109, USA) ,  Arulanantham N. (Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA) ,  France K. (Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Boulder, CO 80303, USA) ,  Serna Javier (Instituto de Astronomia, Universidad Autonoma de Mexico, Ensenada, B.C., Mexico) ,  Hernandez J. (Instituto de Astronomia, Universidad Autonoma de Mexico, Ensenada, B.C., Mexico) ,  Kospal A. (Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Eotvos Lorand Research Network, Konkoly-Thege Miklos ut 15-17, 1121 Budapest, Hungary) ,  Kospal A. (Max Planck Institute for Astronomy, Konigstuhl 17, D-69117 Heidelberg, Germany) ,  Kospal A. (ELTE Eotvos Lorand University, Institute of Physics, Pazmany Peter Setany 1/A, 1117 Budapest, Hungary) ,  Walter F. M. (Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794-3800, USA) ,  Frasca A. (INAF-Osservatorio Astrofisico di Catania, via S. Sofia 78, I-95123, Catania, Italy) ,  Fischer W. J. (Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA) ,  Johns-Krull C. M. (Department of Physics and Astronomy, Rice University, Houston, TX 77005, USA) ,  Schneider P. C. (Hamburger Sternwarte, Gojenbergsweg 112, D-21029 Hamburg, Germany) ,  Robinson C. (Department of Physics and Astronomy, Amherst College, C025 Science Center, 25 East Drive, Amherst, MA 01002, USA) ,  Edwards Suzan (Smith College, Northampton, MA 01063, USA) ,  Abraham P. (Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Eotvos Lorand Research Network, Konkoly-Thege Miklos ut 15-17, 1121 Budapest, Hungary) ,  Abraham P. (ELTE Eotvos Lorand University, Institute of Physics, Pazmany Peter Setany 1/A, 1117 Budapest, Hungary) ,  Fang Min (Purple Mountain Observatory, Chinese Academy of Sciences, 10 Yuanhua Road, Nanjing 210023, People’s Republic of China) ,  Erkal J. (European Southern Observatory, Karl-Schwarzschild-Strasse 2, D-85748 Garching, Germany) ,  Manara C. F. (European Southern Observatory, Karl-Schwarzschild-Strasse 2, D-85748 Garching, Germany) ,  Alcala J. M. (INAF-Osservatorio Astronomico di Capodimonte, via Moiariello 16, I-80131 Naples, Italy) ,  Alecian E. (Universite Grenoble Alpes, CNRS, IPAG, F-38000 Grenoble, France) ,  Alexander R. D. (School of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH, UK) ,  Alonso-Santiago J. (INAF-Osservatorio Astrofisico di Catania, via S. Sofia 78, I-95123, Catania, Italy) ,  Antoniucci Simone (INAF-Osservatorio Astronomico di Roma, via di Frascati 33, I-00078, Monte Porzio Catone, Italy) ,  Ardila David R. (Jet Propulsion Laboratory/California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA) ,  Banzatti Andrea (Department of Physics, Texas State University, San Marcos, TX 78666, USA) ,  Benisty M. (Universite Grenoble Alpes, CNRS, IPAG, F-38000 Grenoble, France) ,  Bergin Edwin A. (Department of Astronomy, University of Michigan, 1085 South University Avenue, Ann Arbor, MI 48109, USA) ,  Biazzo Katia (INAF-Osservatorio Astronomico di Roma, via di Frascati 33, I-00078, Monte Porzio Catone, Italy) ,  Briceno Cesar (Cerro Tololo Inter-American Observatory/NSF’s NOIRLab, Casilla 603, La Serena, Chile) ,  Campbell-White Justyn (SUPA, School of Science and Engineering, University of Dundee, Nethergate, Dundee DD1 4HN, UK) ,  Cleeves L. Ilsedore (Department of Astronomy, University of Virginia, Charlottesville, VA 22904, USA) ,  Coffey Deirdre (School of Physics, University College Dublin, Dublin 4, Ireland) ,  Coffey Deirdre (The Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin 2, Ireland) ,  Eisloffel Jochen (Thueringer Landessternwarte, Sternwarte 5, D-07778 Tautenburg, Germany) ,  Facchini Stefano (European Southern Observatory, Karl-Schwarzschild-Strasse 2, D-85748 Garching, Germany) ,  Fedele D. (INAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, I-10025, Pino Torinese, Italy) ,  Fedele D. (INAF-Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, I-50125, Florence, Italy) ,  Fiorellino Eleonora (Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Eotvos Lorand Research Network, Konkoly-Thege Miklos ut 15-17, 1121 Budapest, Hungary) ,  Fiorellino Eleonora (INAF-Osservatorio Astronomico di Roma, via di Frascati 33, I-00078, Monte Porzio Catone, Italy) ,  Froebrich Dirk (School of Physical Sciences, University of Kent, Canterbury CT2 7NH, UK) ,  Gangi Manuele (INAF-Osservatorio Astronomico di Roma, via di Frascati 33, I-00078, Monte Porzio Catone, Italy) ,  Giannini Teresa (INAF-Osservatorio Astronomico di Roma, via di Frascati 33, I-00078, Monte Porzio Catone, Italy) ,  Grankin K. (Department of Stellar Physics, Crimean Astrophysical Observatory, 298409 Nauchny, Crimea) ,  Guenther Hans Moritz (MIT Kavli Institute for Astrophysics and Space Research, 77 Massachusetts Avenue, Cambridge, MA 02139, USA) ,  Guo Zhen (Centre for Astrophysics Research, University of Hertfordshire, Hatfield AL10 9AB, UK) ,  Hartmann Lee (Department of Astronomy, University of Michigan, 1085 South University Avenue, Ann Arbor, MI 48109, USA) ,  Hillenbrand Lynne A. (Department of Astronomy, California Institute of Technology, 1216 East California Boulevard, Pasadena, CA 91125, USA) ,  Hinton P. C. (Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Boulder, CO 80303, USA) ,  Kastner Joel H. (Chester F. Carlson Center for Imaging Science, School of Physics and Astronomy, and Laboratory for Multiwavelength Astrophysics, Rochester Institute of Technology, Rochester, NY 14623, USA) ,  Koen Chris (Department of Statistics, University of the Western Cape, Private Bag X17, Bellville, 7535, South Africa) ,  Mauco K. (Instituto de Fisica y Astronomia, Facultad de Ciencias, Universidad de Valparaiso, Av. Gran Bretana 1111, 5030 Casilla, Valparaiso, Chile) ,  Mauco K. (Nucleo Milenio de Formacion Planetaria, Universidad de Valparaiso, Av. Gran Bretana 1111, Valparaiso, Chile) ,  Mendigutia I. (Centro de Astrobiologia (CSIC-INTA), ESA-ESAC Campus, E-28692, Villanueva de la Canada, Madrid, Spain) ,  Nisini B. (INAF-Osservatorio Astronomico di Roma, via di Frascati 33, I-00078, Monte Porzio Catone, Italy) ,  Panwar Neelam (Aryabhatta Research Institute of Observational Sciences, Manora Peak, Nainital, Uttarakhand 263001, India) ,  Principe D. A. (MIT Kavli Institute for Astrophysics and Space Research, 77 Massachusetts Avenue, Cambridge, MA 02139, USA) ,  Robberto Massimo (Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA) ,  Robberto Massimo (Johns Hopkins University, 3400 North Charles Street, Baltimore, MD 21218, USA) ,  Sicilia-Aguilar A. (SUPA, School of Science and Engineering, University of Dundee, Nethergate, Dundee DD1 4HN, UK) ,  Valenti Jeff A. (Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA) ,  Wendeborn J. (Institute for Astrophysical Research, Department of Astronomy, Boston University, 725 Commonwealth Avenue, Boston, MA 02215, USA) ,  Williams Jonathan P. (Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, USA) ,  Xu Ziyan (Kavli Institute for Astronomy and Astrophysics, Peking University, Yiheyuan 5, Haidian Qu, 100871 Beijing, People’s Republic of China) ,  Xu Ziyan (Department of Astronomy, Peking University, Yiheyuan 5, Haidian Qu, 100871 Beijing, People’s Republic of China) ,  Yadav R. K. (National Astronomical Research Institute of Thailand, Sirindhorn AstroPark, 260 Moo 4, T. Donkaew, A. Maerim, Chiangmai 50180, Thailand)
資料名： Astronomical Journal  (Astronomical Journal)
巻： 163  号： 3  ページ： 114 (24pp)  発行年： 2022年 
JST資料番号： W1567A  ISSN： 1538-3881  資料種別： 逐次刊行物 (A)
記事区分： 原著論文  発行国： イギリス (GBR)  言語： 英語 (EN)

抄録/ポイント： アタカマ大型ミリメータ/サブミリ波アレイとJames Webb宇宙望遠鏡から来るデータと結合した,低質量プレメインシーケンス星の必須標準(ULLYSES)Director Discretionary ProgramとしてのYoung StarのHubble UV Legcy Libraryは,若年星とそれらの原惑星ディスク間の関係の理解を革命する基礎を提供する。ディスク進化と惑星形成の物理の総合評価は,質量付加,質量流出,およびディスク構造の間の複雑な関係を理解する必要がある。ここでは,ULLYSESスペクトルの調査(ODYSSEUS)調査のための協力と,調査から生じる科学の実証として,Orion OB1bにおける古典的T Tauri Star CVSO 109の初期結果を示す,Young Stars周辺のOutflowsとDisksを記述した。ODYSSEUSはULLYSESスペクトルデータベースを分析し,(1)付加流が降着速度と磁気構造に依存する方法,(2)風と噴流が打ち上げられるか,そして,質量損失速度が降着するかどうか,および(3)惑星形成ディスクの温暖な内部領域の化学に対するFUV放射の影響を確立する。ODYSSEUSは,また,X線,光学,近赤外,およびミリ波で,ULLYSESデータの影響を高めるために,同時観測を取得,提供する。著者らの目標は,プロト惑星ディスクにおける質量付加のレベルと発展,内部ディスク質量損失の特性と大きさ,およびイオン化レベルと駆動ディスク化学を決定するUV放射場の影響を正確に測定するための一貫したフレームワークを提供することである。Please refer to the publisher for the copyright holders. Translated from English into Japanese by JST.【JST・京大機械翻訳】

シソーラス用語： X線 ,  イオン化 ,  *円板 ,  紫外線 ,  惑星 ,  *動機づけ ,  スペクトル ,  近赤外線 ,  EHF波 ,  磁気構造 ,  サブミリ波 ,  惑星進化
準シソーラス用語： 同時観測 ,  惑星形成 ,  質量損失 , 【Automatic Indexing@JST】

分類 (2件)： 恒星  (DB05000P) ,  宇宙線起源  (DB02020Q)

タイトルに関連する用語 (5件)： 調査 ,  動機付け ,  降着 ,  放出 ,  円盤