Issue |
A&A
Volume 685, May 2024
|
|
---|---|---|
Article Number | A75 | |
Number of page(s) | 22 | |
Section | Numerical methods and codes | |
DOI | https://doi.org/10.1051/0004-6361/202346662 | |
Published online | 14 May 2024 |
PDRs4All
IV. An embarrassment of riches: Aromatic infrared bands in the Orion Bar★
1
Department of Physics & Astronomy, The University of Western Ontario,
London
ON
N6A 3K7,
Canada
e-mail: rchown3@uwo.ca
2
Institute for Earth and Space Exploration, The University of Western Ontario,
London
ON
N6A 3K7,
Canada
3
Carl Sagan Center, SETI Institute,
339 Bernardo Avenue, Suite 200,
Mountain View,
CA
94043,
USA
4
Leiden Observatory, Leiden University,
PO Box 9513,
2300 RA
Leiden,
The Netherlands
5
Astronomy Department, University of Maryland,
College Park,
MD
20742,
USA
6
Institut de Recherche en Astrophysique et Planétologie, Université Toulouse III – Paul Sabatier, CNRS, CNES,
9 Av. du colonel Roche,
31028
Toulouse Cedex 04,
France
7
Institut d’Astrophysique Spatiale, Université Paris-Saclay, CNRS,
Bâtiment 121,
91405
Orsay Cedex,
France
8
Department of Astronomy, University of Michigan,
1085 South University Avenue,
Ann Arbor,
MI
48109,
USA
9
Space Telescope Science Institute,
3700 San Martin Drive,
Baltimore,
MD
21218,
USA
10
ACRI-ST, Centre d’Etudes et de Recherche de Grasse (CERGA),
10 Av. Nicolas Copernic,
06130
Grasse,
France
11
INCLASS Common Laboratory,
10 Av. Nicolas Copernic,
06130
Grasse,
France
12
NASA Ames Research Center,
MS 245-6,
Moffett Field,
CA
94035-1000,
USA
13
LERMA, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Université,
92190
Meudon,
France
14
Instituto de Física Fundamental (CSIC),
Calle Serrano 121-123,
28006
Madrid,
Spain
15
Institut des Sciences Moléculaires d’Orsay, CNRS, Université Paris-Saclay,
Bâtiment 520,
91405
Orsay Cedex,
France
16
UK Astronomy Technology Centre, Royal Observatory Edinburgh,
Blackford Hill,
Edinburgh
EH9 3HJ,
UK
17
Observatorio Astronómico Nacional (OAN,IGN),
Alfonso XII, 3,
28014
Madrid,
Spain
18
Sterrenkundig Observatorium, Universiteit Gent,
Krijgslaan 281/S9,
9000
Gent,
Belgium
19
KU Leuven Quantum Solid State Physics (QSP),
Celestijnenlaan 200d –
PO Box 2414,
3001
Leuven,
Belgium
20
Institut de Planétologie et d’Astrophysique de Grenoble (IPAG), Université Grenoble Alpes, CNRS,
38000
Grenoble,
France
21
Institut de Radioastronomie Millimétrique (IRAM),
300 rue de la Piscine,
38406
Saint-Martin-d’Hères,
France
22
I. Physikalisches Institut der Universität zu Köln,
Zülpicher Straße 77,
50937
Köln,
Germany
23
Department of Astronomy, Graduate School of Science, The University of Tokyo,
7-3-1 Bunkyo-ku,
Tokyo
113-0033,
Japan
24
Department of Physics, Faculty of Science and Engineering, Meisei University,
2-1-1 Hodokubo, Hino,
Tokyo
191-8506,
Japan
25
Johns Hopkins University,
3400 N. Charles Street,
Baltimore,
MD
21218,
USA
26
Physikalischer Verein – Gesellschaft für Bildung und Wissenschaft,
Robert-Mayer-Straße 2,
60325
Frankfurt am Main,
Germany
27
Institut für Angewandte Physik. Goethe-Universität Frankfurt,
Max-von-Laue-Str. 1,
60438
Frankfurt am Main,
Germany
28
Department of Space, Earth and Environment, Chalmers University of Technology,
Onsala Space Observatory,
439 92
Onsala,
Sweden
29
Instituto de Astrofísica e Ciências do Espaço,
Tapada da Ajuda, Edifício Leste, 2° Piso,
1349-018
Lisboa,
Portugal
30
Instituto de Física e Química, Universidade Federal de Itajubá,
Av. BPS 1303, Pinheirinho,
37500-903,
Itajubá,
MG,
Brazil
31
Bay Area Environmental Research Institute,
Moffett Field,
CA
94035,
USA
32
Australian Synchrotron, Australian Nuclear Science and Technology Organisation (ANSTO),
800 Blackburn Rd, Clayton, Victoria 3168,
Melbourne,
Australia
33
INAF – Osservatorio Astrofisico di Catania,
Via Santa Sofia 78,
95123
Catania,
Italy
34
Laboratoire de Physique de l’École Normale Supérieure, ENS, Université PSL, CNRS, Sorbonne Université, Université de Paris,
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
FELIX Laboratory, Institute for Molecules and Materials, Radboud University,
Toernooiveld 7,
6525 ED
Nijmegen,
The Netherlands
40
School of Physics, University of Hyderabad,
Hyderabad,
Telangana
500046,
India
41
Department of Earth, Environment, and Physics Worcester State University,
486 Chandler St,
Worcester,
MA
01602,
USA
42
Anton Pannekoek Institute for Astronomy (API), University of Amsterdam,
Science Park 904,
1098 XH
Amsterdam,
The Netherlands
43
Delft University of Technology, Delft,
Mekelweg 5,
2628 CD
Delft,
The Netherlands
44
Laboratoire de Physique des deux infinis Irène Joliot-Curie, Université Paris-Saclay, CNRS/IN2P3,
Bâtiment 104,
91405
Orsay Cedex,
France
45
Department of Chemistry, GITAM school of Science, GITAM Deemed to be University,
NH 207, Nagadenehalli, Doddaballapur taluk,
Bengaluru –
561203,
Karnataka,
India
46
Institut de Physique de Rennes, UMR CNRS 6251,
Université de Rennes 1, Campus de Beaulieu,
35042
Rennes Cedex,
France
47
Department of Chemistry, The University of British Columbia, Vancouver,
2036 Main Mall,
Vancouver,
BC
V6T 1Z1,
Canada
48
National Radio Astronomy Observatory (NRAO),
520 Edgemont Road,
Charlottesville,
VA
22903,
USA
49
European Space Astronomy Centre (ESAC/ESA),
Villanueva de la Cañada,
28692
Madrid,
Spain
50
Observatoire de Paris, PSL University, Sorbonne Université, LERMA,
75014
Paris,
France
51
Harvard-Smithsonian Center for Astrophysics,
60 Garden Street,
Cambridge
MA
02138,
USA
52
Sorbonne Université, CNRS, UMR 7095, Institut d’Astrophysique de Paris,
98bis bd Arago,
75014
Paris,
France
53
Institut Universitaire de France, Ministère de l’Enseignement Supérieur et de la Recherche,
1 rue Descartes,
75231
Paris Cedex 05,
France
54
Department of Physics and Astronomy, Rice University,
Houston
TX,
77005-1892,
USA
55
Yunnan Observatories, Chinese Academy of Sciences,
396 Yangfangwang, Guandu District,
Kunming
650216,
PR China
56
Chinese Academy of Sciences South America Center for Astronomy, National Astronomical Observatories, CAS,
Beijing
100101,
PR China
57
Departments of Chemistry and Astronomy, University of Virginia,
Charlottesville,
Virginia
22904,
USA
58
InterCat and Dept. Physics and Astron., Aarhus University,
Ny Munkegade 120,
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,
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
Institut de Ciencies de l’Espai (ICE, CSIC),
Can Magrans, s/n,
08193
Bellaterra,
Barcelona,
Spain
63
ICREA,
Pg. Lluìs Companys 23,
08010
Barcelona,
Spain
64
Institut d’Estudis Espacials de Catalunya (IEEC),
08034
Barcelona,
Spain
65
European Space Agency, Space Telescope Science Institute,
3700 San Martin Drive,
Baltimore
MD
21218,
USA
66
Institute of Astronomy, Russian Academy of Sciences,
119017,
Pyatnitskaya str. 48,
Moscow,
Russia
67
Department of Earth, Ocean, & Atmospheric Sciences, University of British Columbia,
British Columbia
V6T 1Z4,
Canada
68
Telespazio UK for ESA, ESAC,
28692 Villanueva de la Cañada,
Madrid,
Spain
69
IPAC, California Institute of Technology,
Pasadena,
CA,
USA
70
Department of Physics and Astronomy, University of Missouri,
701 S College Ave,
Columbia,
MO
65211,
USA
71
Max Planck Institute for Astronomy,
Königstuhl 17,
69117
Heidelberg,
Germany
72
Chemical Sciences Division, Lawrence Berkeley National Laboratory,
Berkeley,
CA,
USA
73
Kenneth S. Pitzer Center for Theoretical Chemistry, Department of Chemistry,
420 Latimer Hall, University of California,
Berkeley,
CA
94720-1460,
USA
74
AIM, CEA, CNRS, Université Paris-Saclay, Université Paris Diderot,
Sorbonne Paris Cité,
91191
Gif-sur-Yvette,
France
75
Institut des Sciences Moléculaires, CNRS, Université de Bordeaux,
33405
Talence,
France
76
Department of Chemistry, Massachusetts Institute of Technology,
Cambridge,
MA
02139,
USA
77
Instituto de Ciencia de Materiales de Madrid (CSIC),
Sor Juana Ines de la Cruz 3,
28049,
Madrid,
Spain
78
Department of Physics,
PO Box 64,
00014
University of Helsinki,
Helsinki,
Finland
79
Steward Observatory, University of Arizona,
Tucson,
AZ
85721-0065,
USA
80
BoldlyGo Institute,
31 W 34TH ST FL 7 STE 7159,
New York,
NY
10001,
USA
81
Department of Physics, College of Science, United Arab Emirates University (UAEU),
Al-Ain
15551,
UAE
82
National Astronomical Observatory of Japan, National Institutes of Natural Science,
2-21-1 Osawa, Mitaka,
Tokyo
181-8588,
Japan
83
Sorbonne Université, CNRS, UMR 7095, Institut d’Astrophysique de Paris,
98bis bd Arago,
75014
Paris,
France
84
California Institute of Technology, IPAC,
770, S. Wilson Ave.,
Pasadena,
CA
91125,
USA
85
Department of Physics, Institute of Science, Banaras Hindu University,
Varanasi
221005,
India
86
University of Central Florida,
Orlando,
FL
32765,
USA
87
Van’t Hoff Institute for Molecular Sciences, University of Amsterdam,
PO Box 94157,
1090 GD,
Amsterdam,
The Netherlands
88
Laboratoire de Chimie et Physique Quantiques LCPQ/FERMI, UMR5626, Université de Toulouse (UPS) and CNRS,
Toulouse,
France
89
Laboratory Astrophysics Group of the Max Planck Institute for Astronomy at the Friedrich Schiller University Jena, Institute of Solid State Physics,
Helmholtzweg 3,
07743
Jena,
Germany
90
Instituto de Matemática, Estatística e Física, Universidade Federal do Rio Grande,
96201-900
Rio Grande,
RS,
Brazil
91
Center for Astrophysics and Space Sciences, Department of Physics, University of California,
San Diego, 9500 Gilman Drive,
La Jolla,
CA
92093,
USA
92
School of Chemistry, The University of Nottingham,
University Park,
Nottingham
NG7 2RD,
UK
93
Astronomy Department, Ohio State University,
Columbus,
OH
43210,
USA
94
Space Science Institute,
4765 Walnut St., R203,
Boulder,
CO
80301,
USA
95
Department of Physics, Stockholm University,
10691
Stockholm,
Sweden
96
Department of Physics, Texas State University,
San Marcos,
TX
78666,
USA
97
School of Physics and Astronomy, Sun Yat-sen University,
2 Da Xue Road, Tangjia,
Zhuhai
519000,
Guangdong Province,
PR China
98
Star and Planet Formation Laboratory, RIKEN Cluster for Pioneering Research,
Hirosawa 2-1, Wako,
Saitama
351-0198,
Japan
99
Institute of Deep Space Sciences, Deep Space Exploration Laboratory,
Hefei
230026,
PR China
Received:
14
April
2023
Accepted:
1
August
2023
Context. Mid-infrared observations of photodissociation regions (PDRs) are dominated by strong emission features called aromatic infrared bands (AIBs). The most prominent AIBs are found at 3.3, 6.2, 7.7, 8.6, and 11.2 µm. The most sensitive, highest-resolution infrared spectral imaging data ever taken of the prototypical PDR, the Orion Bar, have been captured by JWST. These high-quality data allow for an unprecedentedly detailed view of AIBs.
Aims. We provide an inventory of the AIBs found in the Orion Bar, along with mid-IR template spectra from five distinct regions in the Bar: the molecular PDR (i.e. the three H2 dissociation fronts), the atomic PDR, and the H II region.
Methods. We used JWST NIRSpec IFU and MIRI MRS observations of the Orion Bar from the JWST Early Release Science Program, PDRs4All (ID: 1288). We extracted five template spectra to represent the morphology and environment of the Orion Bar PDR. We investigated and characterised the AIBs in these template spectra. We describe the variations among them here.
Results. The superb sensitivity and the spectral and spatial resolution of these JWST observations reveal many details of the AIB emission and enable an improved characterization of their detailed profile shapes and sub-components. The Orion Bar spectra are dominated by the well-known AIBs at 3.3, 6.2, 7.7, 8.6, 11.2, and 12.7 µm with well-defined profiles. In addition, the spectra display a wealth of weaker features and sub-components. The widths of many AIBs show clear and systematic variations, being narrowest in the atomic PDR template, but showing a clear broadening in the H II region template while the broadest bands are found in the three dissociation front templates. In addition, the relative strengths of AIB (sub-)components vary among the template spectra as well. All AIB profiles are characteristic of class A sources as designated by Peeters (2022, A&A, 390, 1089), except for the 11.2 µm AIB profile deep in the molecular zone, which belongs to class B11.2. Furthermore, the observations show that the sub-components that contribute to the 5.75, 7.7, and 11.2 µm AIBs become much weaker in the PDR surface layers. We attribute this to the presence of small, more labile carriers in the deeper PDR layers that are photolysed away in the harsh radiation field near the surface. The 3.3/11.2 AIB intensity ratio decreases by about 40% between the dissociation fronts and the H II region, indicating a shift in the polycyclic aromatic hydrocarbon (PAH) size distribution to larger PAHs in the PDR surface layers, also likely due to the effects of photochemistry. The observed broadening of the bands in the molecular PDR is consistent with an enhanced importance of smaller PAHs since smaller PAHs attain a higher internal excitation energy at a fixed photon energy.
Conclusions. Spectral-imaging observations of the Orion Bar using JWST yield key insights into the photochemical evolution of PAHs, such as the evolution responsible for the shift of 11.2 µm AIB emission from class B11.2 in the molecular PDR to class A11.2 in the PDR surface layers. This photochemical evolution is driven by the increased importance of FUV processing in the PDR surface layers, resulting in a “weeding out” of the weakest links of the PAH family in these layers. For now, these JWST observations are consistent with a model in which the underlying PAH family is composed of a few species: the so-called ‘grandPAHs’.
Key words: astrochemistry / infrared: ISM / ISM: molecules / ISM: individual objects: Orion Bar / photon-dominated region (PDR) / techniques: spectroscopic
The 5 template spectra are available at the CDS via anonymous ftp to cdsarc.cds.unistra.fr (130.79.128.5) or via https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/685/A75
© The Authors 2024
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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