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PDRs4All: A JWST Early Release Science Program on Radiative Feedback from Massive Stars
Team:, PI; Berné, Olivier1; Habart, Émilie2; Peeters, Els3,4,5; Team:, Core; Abergel, Alain2; Bergin, Edwin A.6; Bernard-Salas, Jeronimo7,8; Bron, Emeric9; Cami, Jan3,4,5; Dartois, Emmanuel10; Fuente, Asunción11; Goicoechea, Javier R.12; Gordon, Karl D.13,14; Okada, Yoko15; Onaka, Takashi16,17; Robberto, Massimo13,18; Röllig, Markus15; Tielens, Alexander G. G. M.19,20; Vicente, Sílvia21; Wolfire, Mark G.20; Team:, Extended Core; Alarcón, Felipe6; Boersma, C.22; Canin, Amélie1; Chown, Ryan3,4; Dicken, Daniel2; Languignon, David9; Gal, Romane Le1,23,24; Pound, Marc W.20; Trahin, Boris2; Simmer, Thomas2; Sidhu, Ameek3,4; Putte, Dries Van De13; SEPs, One-time co-authors contributed to; Cuadrado, Sara12; Guilloteau, Claire1,25; Maragkoudakis, Alexandros22; Schefter, Bethany R.3; Schirmer, Thiébaut26; Collaborators:; Cazaux, Stéphanie27; Aleman, Isabel28; Allamandola, Louis22,29; Auchettl, Rebecca30; Baratta, Giuseppe Antonio31; Bejaoui, Salma22; Bera, Partha P.22,29; Bilalbegović, Goranka32; Black, John H.33; Boulanger, Francois34; Bouwman, Jordy35,36,37; Brandl, Bernhard19,38; Brechignac, Philippe10; Brünken, Sandra39; Burkhardt, Andrew40; Candian, Alessandra19,41; Cernicharo, Jose13; Chabot, Marin42; Chakraborty, Shubhadip43; Champion, Jason1; Colgan, Sean W. J.44; Cooke, Ilsa R.45; Coutens, Audrey1; Cox, Nick L. J.46; Demyk, Karine1; Meyer, Jennifer Donovan47; Engrand, Cécile42; Foschino, Sacha1; García-Lario, Pedro48; Gavilan, Lisseth22; Gerin, Maryvonne49; Godard, Marie10; Gottlieb, Carl A.50; Guillard, Pierre51,52; Gusdorf, Antoine34,49; Hartigan, Patrick53; He JH(何金华)54,55,56; Herbst, Eric57; Hornekaer, Liv58; Jäger, Cornelia59; Janot-Pacheco, Eduardo60; Joblin, Christine1; Kaufman, Michael61; Kemper, Francisca62,63; Kendrew, Sarah64; Kirsanova, Maria S.65; Klaassen, Pamela66; Knight, Collin3; Kwok, Sun67; Labiano, Álvaro68; Lai, Thomas S.-Y.69; Lee, Timothy J.70; Lefloch, Bertrand23; Petit, Franck Le9; Li, Aigen71; Linz, Hendrik72; Mackie, Cameron J.73,74; Madden, Suzanne C.75; Mascetti, Joëlle76; McGuire, Brett A.77,78; Merino, Pablo79; Micelotta, Elisabetta R.80; Misselt, Karl81; Morse, Jon A.82; Mulas, Giacomo1,83; Neelamkodan, Naslim84,85; Ohsawa, Ryou86; Omont, Alain51; Paladini, Roberta87; Palumbo, Maria Elisabetta31; Pathak, Amit88; Pendleton, Yvonne J.70; Petrignani, Annemieke89; Pino, Thomas10; Puga, Elena90; Rangwala, Naseem44; Rapacioli, Mathias91; Ricca, Alessandra5,22; Roman-Duval, Julia13; Roser, Joseph5,22; Roueff, Evelyne9; Rouillé, Gaël59; Salama, Farid22; Sales, Dinalva A.92; Sandstrom, Karin93; Sarre, Peter94; Sciamma-O'Brien, Ella22; Sellgren, Kris95; Shannon, Matthew J.22; Shenoy, Sachindev S.96; Teyssier, David97; Thomas, Richard D.98; Togi, Aditya99; Verstraete, Laurent2; Witt, Adolf N.100; Wootten, Alwyn47; Ysard, Nathalie2; Zettergren, Henning98; Zhang, Yong101; Zhang, Ziwei E.102; Zhen, Junfeng103
发表期刊PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC
2022-05-01
卷号134期号:1035
DOI10.1088/1538-3873/ac604c
产权排序第54完成单位
收录类别SCI
摘要

Massive stars disrupt their natal molecular cloud material through radiative and mechanical feedback processes. These processes have profound effects on the evolution of interstellar matter in our Galaxy and throughout the universe, from the era of vigorous star formation at redshifts of 1-3 to the present day. The dominant feedback processes can be probed by observations of the Photo-Dissociation Regions (PDRs) where the far-ultraviolet photons of massive stars create warm regions of gas and dust in the neutral atomic and molecular gas. PDR emission provides a unique tool to study in detail the physical and chemical processes that are relevant for most of the mass in inter- and circumstellar media including diffuse clouds, proto-planetary disks, and molecular cloud surfaces, globules, planetary nebulae, and star-forming regions. PDR emission dominates the infrared (IR) spectra of star-forming galaxies. Most of the Galactic and extragalactic observations obtained with the James Webb Space Telescope (JWST) will therefore arise in PDR emission. In this paper we present an Early Release Science program using the MIRI, NIRSpec, and NIRCam instruments dedicated to the observations of an emblematic and nearby PDR: the Orion Bar. These early JWST observations will provide template data sets designed to identify key PDR characteristics in JWST observations. These data will serve to benchmark PDR models and extend them into the JWST era. We also present the Science-Enabling products that we will provide to the community. These template data sets and Science-Enabling products will guide the preparation of future proposals on star-forming regions in our Galaxy and beyond and will facilitate data analysis and interpretation of forthcoming JWST observations.

资助项目STScI under NASA[NAS5-03127] ; STScI under NASA[1288] ; Univ. of Maryland[1288] ; Univ. of Michigan[1288] ; Univ. of Toledo[1288] ; Programme National Physique et Chimie du Milieu Interstellaire (PCMI) of CNRS/INSU ; INC/INP - CEA ; CNES ; APR grants by CNES[6315] ; APR grants by CNES[6410] ; National Science and Engineering Council of Canada (NSERC) Discovery Grant program[RGPIN-2020-06434] ; National Science and Engineering Council of Canada (NSERC) Discovery Grant program[RGPIN-2021-04197] ; Western Strategic Support Accelerator Grant[0000050636] ; Spanish MCINN[PID2019-106110GB-I00] ; Deutsche Forschungsgemeinschaft (DFG)[184018867] ; JSPS Bilateral Program[120219939] ; NASA Astrophysics Data Analysis Program[80NSSC19K0573] ; NASA Ames Research Center through the San Jose State University Research Foundation[NNX17AJ88A] ; Internal Scientist Funding Model (ISFM) Directed Work Package at NASA Ames titled: Laboratory Astrophysics-The NASA Ames PAH IR Spectroscopic Database
项目资助者STScI under NASA[NAS5-03127, 1288] ; Univ. of Maryland[1288] ; Univ. of Michigan[1288] ; Univ. of Toledo[1288] ; Programme National Physique et Chimie du Milieu Interstellaire (PCMI) of CNRS/INSU ; INC/INP - CEA ; CNES ; APR grants by CNES[6315, 6410] ; National Science and Engineering Council of Canada (NSERC) Discovery Grant program[RGPIN-2020-06434, RGPIN-2021-04197] ; Western Strategic Support Accelerator Grant[0000050636] ; Spanish MCINN[PID2019-106110GB-I00] ; Deutsche Forschungsgemeinschaft (DFG)[184018867] ; JSPS Bilateral Program[120219939] ; NASA Astrophysics Data Analysis Program[80NSSC19K0573] ; NASA Ames Research Center through the San Jose State University Research Foundation[NNX17AJ88A] ; Internal Scientist Funding Model (ISFM) Directed Work Package at NASA Ames titled: Laboratory Astrophysics-The NASA Ames PAH IR Spectroscopic Database
语种英语
学科领域天文学 ; 恒星与银河系
文章类型Article
出版者IOP Publishing Ltd
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN0004-6280
URL查看原文
WOS记录号WOS:000804410300001
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]POLYCYCLIC AROMATIC-HYDROCARBONS ; INFRARED-EMISSION BANDS ; ORION BAR REGION ; PHOTODISSOCIATION REGIONS ; PHYSICAL CONDITIONS ; MOLECULAR-HYDROGEN ; INTERSTELLAR DUST ; C-II ; LINE EMISSION ; IR EMISSION
引用统计
被引频次：37[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
版本出版稿
条目标识符http://ir.ynao.ac.cn/handle/114a53/25206
专题其他
通讯作者Team:, PI
作者单位1.Institut de Recherche en Astrophysique et Planétologie, Université de Toulouse, CNRS, CNES, UPS, 9 Av. du colonel Roche, F-31028 Toulouse Cedex 04, France [email protected];
2.Institut d'Astrophysique Spatiale, Université Paris-Saclay, CNRS, Bâtiment 121, F-91405 Orsay Cedex, France;
3.Department of Physics & Astronomy, The University of Western Ontario, London ON N6A 3K7, Canada;
4.Institute for Earth and Space Exploration, The University of Western Ontario, London ON N6A 3K7, Canada;
5.Carl Sagan Center, SETI Institute, 339 Bernardo Avenue, Suite 200, Mountain View, CA 94043, USA;
6.Department of Astronomy, University of Michigan, 1085 South University Avenue, Ann Arbor, MI 48109, USA;
7.ACRI-ST, Centre d'Etudes et de Recherche de Grasse (CERGA), 10 Av. Nicolas Copernic, F-06130 Grasse, France;
8.INCLASS Laboratoire Commun., 10 Av. Nicolas Copernic, 06130 Grasse, France;
9.LERMA, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universités, F-92190 Meudon, France;
10.Institut des Sciences Moléculaires d'Orsay, Université Paris-Saclay, CNRS, Bâtiment 520, F-91405 Orsay Cedex, France;
11.Observatorio Astronómico Nacional (OAN, IGN), Alfonso XII, 3, E-28014 Madrid, Spain;
12.Instituto de Física Fundamental (CSIC), Calle Serrano 121-123, E-28006, Madrid, Spain;
13.Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA;
14.Sterrenkundig Observatorium, Universiteit Gent, Gent, Belgium;
15.I. Physikalisches Institut der Universität zu Köln, Zülpicher Straße 77, D-50937 Köln, Germany;
16.Department of Physics, Faculty of Science and Engineering, Meisei University, 2-1-1 Hodokubo, Hino, Tokyo 191-8506, Japan;
17.Department of Astronomy, Graduate School of Science, The University of Tokyo, 7-3-1 Bunkyo-ku, Tokyo 113-0033, Japan;
18.Johns Hopkins University, 3400 N. Charles Street, Baltimore, MD 21218, USA;
19.Leiden Observatory, Leiden University, P.O. Box 9513, 2300 RA Leiden, The Netherlands;
20.Astronomy Department, University of Maryland, College Park, MD 20742, USA;
21.Instituto de Astrofísica e Ciências do Espaço, Tapada da Ajuda, Edifício Leste, 2° Piso, P-1349-018 Lisboa, Portugal;
22.NASA Ames Research Center, MS 245-6, Moffett Field, CA 94035-1000, USA;
23.Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Université Grenoble Alpes, CNRS, F-38000 Grenoble, France;
24.Institut de Radioastronomie Millimétrique (IRAM), 300 rue de la piscine, F-38406 Saint-Martin d'Hères, France;
25.Institut de Recherche en Informatique de Toulouse, INP-ENSEEIHT, 2 Rue Charles Camichel, F-31071 Toulouse Cedex 07, France;
26.Department of Space, Earth and Environment, Chalmers University of Technology, Onsala Space Observatory, SE-439 92 Onsala, Sweden;
27.Delft University of Technology, Delft, The Netherlands;
28.Instituto de Física e Química, Universidade Federal de Itajubá, Av. BPS 1303, Pinheirinho, 37500-903, Itajubá, MG, Brazil;
29.Bay Area Environmental Research Institute, Moffett Field, CA 94035, USA;
30.Australian Synchrotron, Australian Nuclear Science and Technology Organisation (ANSTO), Victoria, Australia;
31.INAF—Osservatorio Astrofisico di Catania, Via Santa Sofia 78, I-95123 Catania, Italy;
32.Department of Physics, Faculty of Science, University of Zagreb, Bijenička cesta 32, 10000 Zagreb, Croatia;
33.Department of Space, Earth, and Environment, Chalmers University of Technology, Onsala Space Observatory, SE-43992 Onsala, Sweden;
34.Laboratoire de Physique de l'École Normale Supérieure, ENS, Université PSL, CNRS, Sorbonne Université, Université de Paris, F-75005, Paris, France;
35.Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO 80303, USA;
36.Department of Chemistry, University of Colorado, Boulder, CO 80309, USA;
37.Institute for Modeling Plasma, Atmospheres, and Cosmic Dust (IMPACT), University of Colorado, Boulder, CO 80303, USA;
38.Faculty of Aerospace Engineering, Delft University of Technology, Kluyverweg 1, 2629 HS Delft, The Netherlands;
39.Radboud University, Institute for Molecules and Materials, FELIX Laboratory, Toernooiveld 7, 6525 ED Nijmegen, the Netherlands;
40.Department of Physics, Wellesley College, 106 Central Street, Wellesley, MA 02481, USA;
41.TU Library, Delft University of Technology, Prometheusplein 1, 2628 ZC Delft, The Netherlands;
42.Laboratoire de Physique des deux infinis Irène Joliot-Curie, Université Paris-Saclay, CNRS/IN2P3, Bâtiment 104, F-91405 Orsay Cedex, France;
43.Institut de Physique de Rennes, UMR CNRS 6251, Université de Rennes 1, Campus de Beaulieu, F-35042 Rennes Cedex, France;
44.NASA Ames Research Center, Moffett Field, CA 94035, USA;
45.Department of Chemistry, The University of British Columbia, Vancouver, British Columbia, Canada;
46.ACRI-ST, 260 route du Pin Montard, F-06904, Sophia Antipolis, France;
47.National Radio Astronomy Observatory (NRAO), 520 Edgemont Road, Charlottesville, VA 22903, USA;
48.European Space Astronomy Centre (ESAC/ESA), Villanueva de la Cañada, E-28692 Madrid, Spain;
49.Observatoire de Paris, PSL University, Sorbonne Université, LERMA, F-75014, Paris, France;
50.Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge MA 02138, USA;
51.Sorbonne Université, CNRS, UMR 7095, Institut d'Astrophysique de Paris, 98bis bd Arago, F-75014 Paris, France;
52.Institut Universitaire de France, Ministère de l'Enseignement Supérieur et de la Recherche, 1 rue Descartes, F-75231 Paris Cedex 05, France;
53.Department of Physics and Astronomy, Rice University, Houston, TX 77005-1892, USA;
54.Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming, 650216, People's Republic of China;
55.Chinese Academy of Sciences South America Center for Astronomy, National Astronomical Observatories, CAS, Beijing 100101, People's Republic of China;
56.Departamento de Astronomía, Universidad de Chile, Casilla 36-D, Santiago, Chile;
57.Departments of Chemistry and Astronomy, University of Virginia, Charlottesville, VA 22904, USA;
58.InterCat and Dept. Physics and Astron., Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark;
59.Laboratory Astrophysics Group of the Max Planck Institute for Astronomy at the Friedrich Schiller University Jena, Institute of Solid State Physics, Helmholtzweg 3, D-07743 Jena, Germany;
60.Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, 05509-090 São Paulo, SP, Brazil;
61.Department of Physics and Astronomy, San José State University, San Jose, CA 95192, USA;
62.European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748 Garching b. München, Germany;
63.Institute of Astronomy and Astrophysics, Academia Sinica, No. 1, Sec. 4, Roosevelt Rd., Taipei 10617, Taiwan;
64.European Space Agency, Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA;
65.Institute of Astronomy, Russian Academy of Sciences, 119017, Pyatnitskaya str., 48 , Moscow, Russia;
66.UK Astronomy Technology Centre, Royal Observatory Edinburgh, Blackford Hill EH9 3HJ, UK;
67.Department of Earth, Ocean, & Atmospheric Sciences, University of British Columbia, V6T 1Z4, Canada;
68.Telespazio UK for ESA, ESAC, E-28692 Villanueva de la Cañada, Madrid, Spain;
69.IPAC, California Institute of Technology, Pasadena, CA, USA;
70.NASA Ames Research Center, MS 245-3, Moffett Field, CA 94035-1000, USA;
71.Department of Physics and Astronomy, University of Missouri, Columbia, MO 65211, USA;
72.Max Planck Institute for Astronomy, Königstuhl 17, D-69117 Heidelberg, Germany;
73.Chemical Sciences Division, Lawrence Berkeley National Laboratory, Berkeley, CA, USA;
74.Kenneth S. Pitzer Center for Theoretical Chemistry, Department of Chemistry, University of California—Berkeley, Berkeley, CA, USA;
75.AIM, CEA, CNRS, Université Paris-Saclay, Université Paris Diderot, Sorbonne Paris Cité, F-91191 Gif-sur-Yvette, France;
76.Institut des Sciences Moléculaires, CNRS, Université de Bordeaux, F-33405 Talence, France;
77.Department of Chemistry, Massachusetts Institute of Technology, Cambridge, MA 02139, USA;
78.National Radio Astronomy Observatory, Charlottesville, VA 22903, USA;
79.Instituto de Ciencia de Materiales de Madrid (CSIC), Sor Juana Ines de la Cruz 3, E-28049, Madrid, Spain;
80.Department of Physics, P.O. Box 64, FI-00014 University of Helsinki, Finland;
81.Steward Observatory, University of Arizona, Tucson, AZ 85721-0065, USA;
82.BoldlyGo Institute, 31 W 34TH ST FL 7 STE 7159, New York, NY 10001, USA;
83.INAF—Osservatorio Astronomico di Cagliari, via della scienza 5, I-09047 Selargius, Italy;
84.Department of Physics, College of Science, United Arab Emirates University (UAEU), Al-Ain, 15551, UAE;
85.National Astronomical Observatory of Japan, National Institutes of Natural Science, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan;
86.Institute of Astronomy, Graduate School of Science, The University of Tokyo, 2-21-1, Osawa, Mitaka, Tokyo 181-0015, Japan;
87.California Institute of Technology, IPAC, 770, S. Wilson Ave., Pasadena, CA 91125, USA;
88.Department of Physics, Institute of Science, Banaras Hindu University, Varanasi 221005, India;
89.Van't Hoff Institute for Molecular Sciences, University of Amsterdam, P.O. Box 94157, 1090 GD, Amsterdam, The Netherlands;
90.European Space Agency (ESA), ESA Office, Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA;
91.Laboratoire de Chimie et Physique Quantiques LCPQ/IRSAMC, UMR5626, Université de Toulouse (UPS) and CNRS, Toulouse, France;
92.Instituto de Matemática, Estatística e Física, Universidade Federal do Rio Grande, 96201-900, Rio Grande, RS, Brazil;
93.Center for Astrophysics and Space Sciences, Department of Physics, University of California, San Diego, 9500 Gilman Drive, La Jolla, CA 92093, USA;
94.School of Chemistry, The University of Nottingham, University Park, Nottingham, NG7 2RD, UK;
95.Astronomy Department, Ohio State University, Columbus, OH 43210, USA;
96.Space Science Institute, 4765 Walnut St., R203, Boulder, CO 80301, USA;
97.Telespazio Vega UK Ltd for European Space Agency (ESA), Camino bajo del Castillo, s/n, Urbanizacion Villafranca del Castillo, Villanueva de la Cañada, E-28692 Madrid, Spain;
98.Department of Physics, Stockholm University, SE-10691 Stockholm, Sweden;
99.Department of Physics, Texas State University, San Marcos, TX 78666, USA;
100.Ritter Astrophysical Research Center, University of Toledo, Toledo, OH 43606, USA;
101.School of Physics and Astronomy, Sun Yat-sen University, 2 Da Xue Road, Tangjia, Zhuhai 519000, Guangdong Province, People's Republic of China;
102.Star and Planet Formation Laboratory, RIKEN Cluster for Pioneering Research, Wako, Saitama 351-0198, Japan;
103.University of Science and Technology of China, CAS Key Laboratory of Crust-Mantle Materials and Environment, Hefei, Anhui 230026, People's Republic of China
推荐引用方式
GB/T 7714		 Team:, PI,Berné, Olivier,Habart, Émilie,et al. PDRs4All: A JWST Early Release Science Program on Radiative Feedback from Massive Stars[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC,2022,134(1035).
APA Team:, PI.,Berné, Olivier.,Habart, Émilie.,Peeters, Els.,Team:, Core.,...&Zhen, Junfeng.(2022).PDRs4All: A JWST Early Release Science Program on Radiative Feedback from Massive Stars.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC,134(1035).
MLA Team:, PI,et al."PDRs4All: A JWST Early Release Science Program on Radiative Feedback from Massive Stars".PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC 134.1035(2022).
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