Edge-On Disk Study (EODS) Article Swipe
A. Dutrey
,
O. Denis-Alpizar
,
S. Guilloteau
,
C. Foucher
,
S. Gavino
,
D. Semenov
,
V. Piétu
,
E. Chapillon
,
L. Testi
,
E. Dartois
,
E. DiFolco
,
K. Furuya
,
U. Gorti
,
Nicolas Grosso
,
Th. Henning
,
J. M. Huré
,
Á Kóspál
,
F. Le Petit
,
L Majumdar
,
R Meshaka
,
H Nomura
,
N. T. Phuong
,
M. Ruaud
,
Y.W. Tang
,
S Wolf
·
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.1051/0004-6361/202555641
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.1051/0004-6361/202555641
Context . Investigating the vertical distribution of molecular content in protoplanetary disks remains difficult in most disks mildly inclined along the line of sight. In contrast, edge-on disks provide a direct (tomographic) view of the 2D molecular brightness. Aims . We study the radial and vertical molecular distribution as well as the gas temperature and density by observing the Keplerian edge-on disk surrounding the Flying Saucer, a Class II object located in Ophiuchus. Methods . We used new and archival ALMA data to perform a tomography of 12 CO, 13 CO, C 18 O, CN, HCN, CS, H 2 CO, c-C 3 H 2 , N 2 D + , DCN, and 13 CS. We analyzed molecular tomographies and modeled data using the radiative transfer code D ISK F IT . Results . We directly measured the altitude above the mid-plane for each observed species. For the first time, we unambiguously demonstrate the presence of a common molecular layer and measure its thickness. Most molecules are located at the same altitude versus radius. Beyond CO, as predicted by chemical models, the CN emission traces the upper boundary of the molecular layer, whereas the deuterated species (DCN and N 2 D + ) reside below one scale height. Our best fits from D ISK F IT show that most observed transitions in the molecular layer are thermalized because their excitation temperature is the same, around ~17-20K. Conclusions . These long-integration observations clearly reveal a molecular layer predominantly located around one to two scale heights at a temperature above the CO freeze-out temperature. The deuterated molecules are closer to the mid-plane, and N 2 D + may be a good proxy for the CO snowline. Some molecules, such as CN and H 2 CO, are likely influenced by the disk environment, at least beyond the millimeter dust disk radius. The direct observation of the molecular stratification opens the door to detailed chemical modeling in a disk that appears representative of T Tauri disks.
Related Topics
Concepts
Physics
Astrophysics
Radiative transfer
Scale height
Line (geometry)
Excitation temperature
Molecular cloud
Protoplanetary disk
Excitation
Altitude (triangle)
Deuterium
Emission spectrum
Boundary layer
Molecular physics
Spectral line
Layer (electronics)
Atomic physics
Scale (ratio)
Molecule
Spatial distribution
Maser
Protostar
Astrochemistry
Line-of-sight
Atmospheric radiative transfer codes
Boundary (topology)
Mean kinetic temperature
Herbig–Haro object
Electron density
Radiation
Measure (data warehouse)
Photodissociation
Computational physics
Metadata
- Type
- article
- Landing Page
- https://doi.org/10.1051/0004-6361/202555641
- https://www.aanda.org/articles/aa/pdf/2025/12/aa55641-25.pdf
- OA Status
- hybrid
- References
- 51
- OpenAlex ID
- https://openalex.org/W7106654682
All OpenAlex metadata
Raw OpenAlex JSON
- OpenAlex ID
-
https://openalex.org/W7106654682Canonical identifier for this work in OpenAlex
- DOI
-
https://doi.org/10.1051/0004-6361/202555641Digital Object Identifier
- Title
-
Edge-On Disk Study (EODS)Work title
- Type
-
articleOpenAlex work type
- Publication year
-
2025Year of publication
- Publication date
-
2025-11-26Full publication date if available
- Authors
-
A. Dutrey, O. Denis-Alpizar, S. Guilloteau, C. Foucher, S. Gavino, D. Semenov, V. Piétu, E. Chapillon, L. Testi, E. Dartois, E. DiFolco, K. Furuya, U. Gorti, Nicolas Grosso, Th. Henning, J. M. Huré, Á Kóspál, F. Le Petit, L Majumdar, R Meshaka, H Nomura, N. T. Phuong, M. Ruaud, Y.W. Tang, S WolfList of authors in order
- Landing page
-
https://doi.org/10.1051/0004-6361/202555641Publisher landing page
- PDF URL
-
https://www.aanda.org/articles/aa/pdf/2025/12/aa55641-25.pdfDirect link to full text PDF
- Open access
-
YesWhether a free full text is available
- OA status
-
hybridOpen access status per OpenAlex
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https://www.aanda.org/articles/aa/pdf/2025/12/aa55641-25.pdfDirect OA link when available
- Concepts
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Physics, Astrophysics, Radiative transfer, Scale height, Line (geometry), Excitation temperature, Molecular cloud, Protoplanetary disk, Excitation, Altitude (triangle), Deuterium, Emission spectrum, Boundary layer, Molecular physics, Spectral line, Layer (electronics), Atomic physics, Scale (ratio), Molecule, Spatial distribution, Maser, Protostar, Astrochemistry, Line-of-sight, Atmospheric radiative transfer codes, Boundary (topology), Mean kinetic temperature, Herbig–Haro object, Electron density, Radiation, Measure (data warehouse), Photodissociation, Computational physicsTop concepts (fields/topics) attached by OpenAlex
- Cited by
-
0Total citation count in OpenAlex
- References (count)
-
51Number of works referenced by this work
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| abstract_inverted_index.is | 230 |
| abstract_inverted_index.of | 6, 22, 33, 86, 154, 187, 310, 327 |
| abstract_inverted_index.to | 82, 249, 266, 317 |
| abstract_inverted_index.we | 149 |
| abstract_inverted_index.CN, | 94 |
| abstract_inverted_index.CO, | 88, 90, 99, 174, 291 |
| abstract_inverted_index.CS, | 96 |
| abstract_inverted_index.CS. | 113 |
| abstract_inverted_index.For | 145 |
| abstract_inverted_index.ISK | 127, 212 |
| abstract_inverted_index.Our | 207 |
| abstract_inverted_index.The | 261, 307 |
| abstract_inverted_index.and | 44, 54, 78, 111, 118, 159, 196, 269, 288 |
| abstract_inverted_index.are | 165, 224, 264, 292 |
| abstract_inverted_index.c-C | 100 |
| abstract_inverted_index.for | 141, 279 |
| abstract_inverted_index.gas | 52 |
| abstract_inverted_index.its | 161 |
| abstract_inverted_index.may | 274 |
| abstract_inverted_index.new | 77 |
| abstract_inverted_index.one | 204, 248 |
| abstract_inverted_index.the | 3, 20, 34, 42, 51, 58, 63, 122, 136, 139, 146, 152, 168, 180, 184, 188, 192, 221, 231, 257, 267, 280, 296, 302, 311, 315 |
| abstract_inverted_index.two | 250 |
| abstract_inverted_index.(DCN | 195 |
| abstract_inverted_index.ALMA | 80 |
| abstract_inverted_index.Aims | 38 |
| abstract_inverted_index.DCN, | 110 |
| abstract_inverted_index.HCN, | 95 |
| abstract_inverted_index.Most | 163 |
| abstract_inverted_index.Some | 283 |
| abstract_inverted_index.best | 208 |
| abstract_inverted_index.code | 125 |
| abstract_inverted_index.data | 81, 120 |
| abstract_inverted_index.disk | 61, 297, 305, 323 |
| abstract_inverted_index.door | 316 |
| abstract_inverted_index.dust | 304 |
| abstract_inverted_index.each | 142 |
| abstract_inverted_index.fits | 209 |
| abstract_inverted_index.from | 210 |
| abstract_inverted_index.good | 277 |
| abstract_inverted_index.line | 21 |
| abstract_inverted_index.most | 15, 217 |
| abstract_inverted_index.same | 169 |
| abstract_inverted_index.show | 215 |
| abstract_inverted_index.such | 285 |
| abstract_inverted_index.that | 216, 324 |
| abstract_inverted_index.used | 76 |
| abstract_inverted_index.view | 32 |
| abstract_inverted_index.well | 49 |
| abstract_inverted_index.Class | 67 |
| abstract_inverted_index.Tauri | 329 |
| abstract_inverted_index.These | 237 |
| abstract_inverted_index.above | 138, 256 |
| abstract_inverted_index.along | 19 |
| abstract_inverted_index.below | 203 |
| abstract_inverted_index.disks | 11, 16, 27 |
| abstract_inverted_index.first | 147 |
| abstract_inverted_index.layer | 158, 223, 244 |
| abstract_inverted_index.least | 300 |
| abstract_inverted_index.opens | 314 |
| abstract_inverted_index.proxy | 278 |
| abstract_inverted_index.same, | 232 |
| abstract_inverted_index.scale | 205, 251 |
| abstract_inverted_index.study | 41 |
| abstract_inverted_index.their | 227 |
| abstract_inverted_index.time, | 148 |
| abstract_inverted_index.upper | 185 |
| abstract_inverted_index.using | 121 |
| abstract_inverted_index.Beyond | 173 |
| abstract_inverted_index.Flying | 64 |
| abstract_inverted_index.around | 233, 247 |
| abstract_inverted_index.beyond | 301 |
| abstract_inverted_index.closer | 265 |
| abstract_inverted_index.common | 156 |
| abstract_inverted_index.direct | 30, 308 |
| abstract_inverted_index.disks. | 330 |
| abstract_inverted_index.layer, | 190 |
| abstract_inverted_index.likely | 293 |
| abstract_inverted_index.mildly | 17 |
| abstract_inverted_index.object | 69 |
| abstract_inverted_index.radial | 43 |
| abstract_inverted_index.reside | 202 |
| abstract_inverted_index.reveal | 241 |
| abstract_inverted_index.sight. | 23 |
| abstract_inverted_index.traces | 183 |
| abstract_inverted_index.versus | 171 |
| abstract_inverted_index.Context | 0 |
| abstract_inverted_index.Methods | 73 |
| abstract_inverted_index.Results | 131 |
| abstract_inverted_index.Saucer, | 65 |
| abstract_inverted_index.appears | 325 |
| abstract_inverted_index.because | 226 |
| abstract_inverted_index.clearly | 240 |
| abstract_inverted_index.content | 8 |
| abstract_inverted_index.density | 55 |
| abstract_inverted_index.edge-on | 26, 60 |
| abstract_inverted_index.height. | 206 |
| abstract_inverted_index.heights | 252 |
| abstract_inverted_index.located | 70, 166, 246 |
| abstract_inverted_index.measure | 160 |
| abstract_inverted_index.modeled | 119 |
| abstract_inverted_index.models, | 179 |
| abstract_inverted_index.perform | 83 |
| abstract_inverted_index.provide | 28 |
| abstract_inverted_index.radius. | 172, 306 |
| abstract_inverted_index.remains | 12 |
| abstract_inverted_index.species | 194 |
| abstract_inverted_index.whereas | 191 |
| abstract_inverted_index.altitude | 137, 170 |
| abstract_inverted_index.analyzed | 115 |
| abstract_inverted_index.archival | 79 |
| abstract_inverted_index.boundary | 186 |
| abstract_inverted_index.chemical | 178, 319 |
| abstract_inverted_index.detailed | 318 |
| abstract_inverted_index.directly | 134 |
| abstract_inverted_index.emission | 182 |
| abstract_inverted_index.inclined | 18 |
| abstract_inverted_index.measured | 135 |
| abstract_inverted_index.modeling | 320 |
| abstract_inverted_index.observed | 143, 218 |
| abstract_inverted_index.presence | 153 |
| abstract_inverted_index.species. | 144 |
| abstract_inverted_index.transfer | 124 |
| abstract_inverted_index.vertical | 4, 45 |
| abstract_inverted_index.~17-20K. | 234 |
| abstract_inverted_index.Keplerian | 59 |
| abstract_inverted_index.contrast, | 25 |
| abstract_inverted_index.difficult | 13 |
| abstract_inverted_index.mid-plane | 140 |
| abstract_inverted_index.molecular | 7, 36, 46, 116, 157, 189, 222, 243, 312 |
| abstract_inverted_index.molecules | 164, 263 |
| abstract_inverted_index.observing | 57 |
| abstract_inverted_index.predicted | 176 |
| abstract_inverted_index.radiative | 123 |
| abstract_inverted_index.snowline. | 282 |
| abstract_inverted_index.Ophiuchus. | 72 |
| abstract_inverted_index.deuterated | 193, 262 |
| abstract_inverted_index.excitation | 228 |
| abstract_inverted_index.freeze-out | 259 |
| abstract_inverted_index.influenced | 294 |
| abstract_inverted_index.mid-plane, | 268 |
| abstract_inverted_index.millimeter | 303 |
| abstract_inverted_index.molecules, | 284 |
| abstract_inverted_index.thickness. | 162 |
| abstract_inverted_index.tomography | 85 |
| abstract_inverted_index.Conclusions | 235 |
| abstract_inverted_index.brightness. | 37 |
| abstract_inverted_index.demonstrate | 151 |
| abstract_inverted_index.observation | 309 |
| abstract_inverted_index.surrounding | 62 |
| abstract_inverted_index.temperature | 53, 229, 255 |
| abstract_inverted_index.thermalized | 225 |
| abstract_inverted_index.transitions | 219 |
| abstract_inverted_index.distribution | 5, 47 |
| abstract_inverted_index.environment, | 298 |
| abstract_inverted_index.observations | 239 |
| abstract_inverted_index.temperature. | 260 |
| abstract_inverted_index.tomographies | 117 |
| abstract_inverted_index.(tomographic) | 31 |
| abstract_inverted_index.Investigating | 2 |
| abstract_inverted_index.predominantly | 245 |
| abstract_inverted_index.unambiguously | 150 |
| abstract_inverted_index.protoplanetary | 10 |
| abstract_inverted_index.representative | 326 |
| abstract_inverted_index.stratification | 313 |
| abstract_inverted_index.long-integration | 238 |
| cited_by_percentile_year | |
| countries_distinct_count | 13 |
| institutions_distinct_count | 25 |
| citation_normalized_percentile |