%0 Generic %1 habart2023pdrs4all %A Habart, Emilie %A Peeters, Els %A Berné, Olivier %A Trahin, Boris %A Canin, Amélie %A Chown, Ryan %A Sidhu, Ameek %A Van De Putte, Dries %A Alarcón, Felipe %A Schroetter, Ilane %A Dartois, Emmanuel %A Vicente, Sílvia %A Abergel, Alain %A Bergin, Edwin A. %A Bernard-Salas, Jeronimo %A Boersma, Christiaan %A Bron, Emeric %A Cami, Jan %A Cuadrado, Sara %A Dicken, Daniel %A Elyajouri, Meriem %A Fuente, Asunción %A Goicoechea, Javier R. %A Gordon, Karl D. %A Issa, Lina %A Joblin, Christine %A Kannavou, Olga %A Khan, Baria %A Lacinbala, Ozan %A Languignon, David %A Gal, Romane Le %A Maragkoudakis, Alexandros %A Meshaka, Raphael %A Okada, Yoko %A Onaka, Takashi %A Pasquini, Sofia %A Pound, Marc W. %A Robberto, Massimo %A Röllig, Markus %A Schefter, Bethany %A Schirmer, Thiébaut %A Tabone, Benoit %A Tielens, Alexander G. G. M. %A Wolfire, Mark G. %A Zannese, Marion %A Ysard, Nathalie %A Miville-Deschenes, Marc-Antoine %A Aleman, Isabel %A Allamandola, Louis %A Auchettl, Rebecca %A Baratta, Giuseppe Antonio %A Bejaoui, Salma %A Bera, Partha P. %A Black, John H. %A Boulanger, Francois %A Bouwman, Jordy %A Brandl, Bernhard %A Brechignac, Philippe %A Brünken, Sandra %A Buragohain, Mridusmita %A Burkhardt, rew %A Candian, Alessandra %A Cazaux, Stéphanie %A Cernicharo, Jose %A Chabot, Marin %A Chakraborty, Shubhadip %A Champion, Jason %A Colgan, Sean W. J. %A Cooke, Ilsa R. %A Coutens, Audrey %A Cox, Nick L. J. %A Demyk, Karine %A Meyer, Jennifer Donovan %A Foschino, Sacha %A García-Lario, Pedro %A Gavilan, Lisseth %A Gerin, Maryvonne %A Gottlieb, Carl A. %A Guillard, Pierre %A Gusdorf, Antoine %A Hartigan, Patrick %A He, Jinhua %A Herbst, Eric %A Hornekaer, Liv %A Jäger, Cornelia %A Janot-Pacheco, Eduardo %A Kaufman, Michael %A Kemper, Francisca %A Kendrew, Sarah %A Kirsanova, Maria S. %A Klaassen, Pamela %A Kwok, Sun %A Labiano, Álvaro %A Lai, Thomas S. Y. %A Lee, Timothy J. %A Lefloch, Bertrand %A Petit, Franck Le %A Li, Aigen %A Linz, Hendrik %A Mackie, Cameron J. %A Madden, Suzanne C. %A Mascetti, Joëlle %A McGuire, Brett A. %A Merino, Pablo %A Micelotta, Elisabetta R. %A Misselt, Karl %A Morse, Jon A. %A Mulas, Giacomo %A Neelamkodan, Naslim %A Ohsawa, Ryou %A Omont, Alain %A Paladini, Roberta %A Palumbo, Maria Elisabetta %A Pathak, Amit %A Pendleton, Yvonne J. %A Petrignani, Annemieke %A Pino, Thomas %A Puga, Elena %A Rangwala, Naseem %A Rapacioli, Mathias %A Ricca, Alessandra %A Roman-Duval, Julia %A Roser, Joseph %A Roueff, Evelyne %A Rouillé, Gaël %A Salama, Farid %A Sales, Dinalva A. %A Sandstrom, Karin %A Sarre, Peter %A Sciamma-O'Brien, Ella %A Sellgren, Kris %A Shenoy, Sachindev S. %A Teyssier, David %A Thomas, Richard D. %A Togi, Aditya %A Verstraete, Laurent %A Witt, Adolf N. %A Wootten, Alwyn %A Zettergren, Henning %A Zhang, Yong %A Zhang, Ziwei E. %A Zhen, Junfeng %D 2023 %K astrophysics %T PDRs4All II: JWST's NIR and MIR imaging view of the Orion Nebula %U http://arxiv.org/abs/2308.16732 %X The JWST has captured the most detailed and sharpest infrared images ever taken of the inner region of the Orion Nebula, the nearest massive star formation region, and a prototypical highly irradiated dense photo-dissociation region (PDR). We investigate the fundamental interaction of far-ultraviolet photons with molecular clouds. The transitions across the ionization front (IF), dissociation front (DF), and the molecular cloud are studied at high-angular resolution. These transitions are relevant to understanding the effects of radiative feedback from massive stars and the dominant physical and chemical processes that lead to the IR emission that JWST will detect in many Galactic and extragalactic environments. Due to the proximity of the Orion Nebula and the unprecedented angular resolution of JWST, these data reveal that the molecular cloud borders are hyper structured at small angular scales of 0.1-1" (0.0002-0.002 pc or 40-400 au at 414 pc). A diverse set of features are observed such as ridges, waves, globules and photoevaporated protoplanetary disks. At the PDR atomic to molecular transition, several bright features are detected that are associated with the highly irradiated surroundings of the dense molecular condensations and embedded young star. Toward the Orion Bar PDR, a highly sculpted interface is detected with sharp edges and density increases near the IF and DF. This was predicted by previous modeling studies, but the fronts were unresolved in most tracers. A complex, structured, and folded DF surface was traced by the H2 lines. This dataset was used to revisit the commonly adopted 2D PDR structure of the Orion Bar. JWST provides us with a complete view of the PDR, all the way from the PDR edge to the substructured dense region, and this allowed us to determine, in detail, where the emission of the atomic and molecular lines, aromatic bands, and dust originate.

@misc{habart2023pdrs4all, abstract = {The JWST has captured the most detailed and sharpest infrared images ever taken of the inner region of the Orion Nebula, the nearest massive star formation region, and a prototypical highly irradiated dense photo-dissociation region (PDR). We investigate the fundamental interaction of far-ultraviolet photons with molecular clouds. The transitions across the ionization front (IF), dissociation front (DF), and the molecular cloud are studied at high-angular resolution. These transitions are relevant to understanding the effects of radiative feedback from massive stars and the dominant physical and chemical processes that lead to the IR emission that JWST will detect in many Galactic and extragalactic environments. Due to the proximity of the Orion Nebula and the unprecedented angular resolution of JWST, these data reveal that the molecular cloud borders are hyper structured at small angular scales of 0.1-1" (0.0002-0.002 pc or 40-400 au at 414 pc). A diverse set of features are observed such as ridges, waves, globules and photoevaporated protoplanetary disks. At the PDR atomic to molecular transition, several bright features are detected that are associated with the highly irradiated surroundings of the dense molecular condensations and embedded young star. Toward the Orion Bar PDR, a highly sculpted interface is detected with sharp edges and density increases near the IF and DF. This was predicted by previous modeling studies, but the fronts were unresolved in most tracers. A complex, structured, and folded DF surface was traced by the H2 lines. This dataset was used to revisit the commonly adopted 2D PDR structure of the Orion Bar. JWST provides us with a complete view of the PDR, all the way from the PDR edge to the substructured dense region, and this allowed us to determine, in detail, where the emission of the atomic and molecular lines, aromatic bands, and dust originate.}, added-at = {2023-09-04T09:14:40.000+0200}, author = {Habart, Emilie and Peeters, Els and Berné, Olivier and Trahin, Boris and Canin, Amélie and Chown, Ryan and Sidhu, Ameek and Van De Putte, Dries and Alarcón, Felipe and Schroetter, Ilane and Dartois, Emmanuel and Vicente, Sílvia and Abergel, Alain and Bergin, Edwin A. and Bernard-Salas, Jeronimo and Boersma, Christiaan and Bron, Emeric and Cami, Jan and Cuadrado, Sara and Dicken, Daniel and Elyajouri, Meriem and Fuente, Asunción and Goicoechea, Javier R. and Gordon, Karl D. and Issa, Lina and Joblin, Christine and Kannavou, Olga and Khan, Baria and Lacinbala, Ozan and Languignon, David and Gal, Romane Le and Maragkoudakis, Alexandros and Meshaka, Raphael and Okada, Yoko and Onaka, Takashi and Pasquini, Sofia and Pound, Marc W. and Robberto, Massimo and Röllig, Markus and Schefter, Bethany and Schirmer, Thiébaut and Tabone, Benoit and Tielens, Alexander G. G. M. and Wolfire, Mark G. and Zannese, Marion and Ysard, Nathalie and Miville-Deschenes, Marc-Antoine and Aleman, Isabel and Allamandola, Louis and Auchettl, Rebecca and Baratta, Giuseppe Antonio and Bejaoui, Salma and Bera, Partha P. and Black, John H. and Boulanger, Francois and Bouwman, Jordy and Brandl, Bernhard and Brechignac, Philippe and Brünken, Sandra and Buragohain, Mridusmita and Burkhardt, rew and Candian, Alessandra and Cazaux, Stéphanie and Cernicharo, Jose and Chabot, Marin and Chakraborty, Shubhadip and Champion, Jason and Colgan, Sean W. J. and Cooke, Ilsa R. and Coutens, Audrey and Cox, Nick L. J. and Demyk, Karine and Meyer, Jennifer Donovan and Foschino, Sacha and García-Lario, Pedro and Gavilan, Lisseth and Gerin, Maryvonne and Gottlieb, Carl A. and Guillard, Pierre and Gusdorf, Antoine and Hartigan, Patrick and He, Jinhua and Herbst, Eric and Hornekaer, Liv and Jäger, Cornelia and Janot-Pacheco, Eduardo and Kaufman, Michael and Kemper, Francisca and Kendrew, Sarah and Kirsanova, Maria S. and Klaassen, Pamela and Kwok, Sun and Labiano, Álvaro and Lai, Thomas S. Y. and Lee, Timothy J. and Lefloch, Bertrand and Petit, Franck Le and Li, Aigen and Linz, Hendrik and Mackie, Cameron J. and Madden, Suzanne C. and Mascetti, Joëlle and McGuire, Brett A. and Merino, Pablo and Micelotta, Elisabetta R. and Misselt, Karl and Morse, Jon A. and Mulas, Giacomo and Neelamkodan, Naslim and Ohsawa, Ryou and Omont, Alain and Paladini, Roberta and Palumbo, Maria Elisabetta and Pathak, Amit and Pendleton, Yvonne J. and Petrignani, Annemieke and Pino, Thomas and Puga, Elena and Rangwala, Naseem and Rapacioli, Mathias and Ricca, Alessandra and Roman-Duval, Julia and Roser, Joseph and Roueff, Evelyne and Rouillé, Gaël and Salama, Farid and Sales, Dinalva A. and Sandstrom, Karin and Sarre, Peter and Sciamma-O'Brien, Ella and Sellgren, Kris and Shenoy, Sachindev S. and Teyssier, David and Thomas, Richard D. and Togi, Aditya and Verstraete, Laurent and Witt, Adolf N. and Wootten, Alwyn and Zettergren, Henning and Zhang, Yong and Zhang, Ziwei E. and Zhen, Junfeng}, biburl = {https://www.bibsonomy.org/bibtex/297cf535e3fa0c84ea8ebdc887f0832ae/fboulang}, description = {PDRs4All II: JWST's NIR and MIR imaging view of the Orion Nebula}, interhash = {271959820fa419cadc7a7f930e269964}, intrahash = {97cf535e3fa0c84ea8ebdc887f0832ae}, keywords = {astrophysics}, note = {cite arxiv:2308.16732}, timestamp = {2023-09-04T09:14:40.000+0200}, title = {PDRs4All II: JWST's NIR and MIR imaging view of the Orion Nebula}, url = {http://arxiv.org/abs/2308.16732}, year = 2023 }