The GRAVITY young stellar object survey Article Swipe
V. Ganci
,
Lucas Labadie
,
K. Perraut
,
A. Wojtczak
,
J. Kaufhold
,
M. Benisty
,
E. Alécian
,
G. Bourdarot
,
W. Brandner
,
A. Caratti o Garatti
,
C. Dougados
,
R. García López
,
J. Sánchez-Bermúdez
,
A. Soulain
,
A. Amorim
,
Jean-Philippe Berger
,
P. Caselli
,
Y. Clénet
,
A. Drescher
,
A. Eckart
,
F. Eisenhauer
,
M. Fabricius
,
H. Feuchtgruber
,
P. García
,
É. Gendron
,
R. Genzel
,
S. Gillessen
,
Sierra L. Grant
,
G. Heißel
,
Thomas Henning
,
M. Horrobin
,
L. Jocou
,
P. Kervella
,
S. Lacour
,
V. Lapeyrère
,
J.-B. Le Bouquin
,
Pierre Léna
,
D. Lutz
,
F. Mang
,
Nuno Morujão
,
T. Ott
,
T. Paumard
,
G. Perrin
,
D. Ribeiro
,
M. S. Bordoni
,
S. Scheithauer
,
J. Shangguan
,
Thomas Shimizu
,
C. Straubmeier
,
E. Sturm
,
L. J. Tacconi
,
E. F. van Dishoeck
,
F. Vincent
,
J. Woillez
·
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.1051/0004-6361/202346926
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.1051/0004-6361/202346926
Context . Temporal variability in the photometric and spectroscopic properties of protoplanetary disks is common in young stellar objects. However, evidence pointing toward changes in their morphology over short timescales has only been found for a few sources, mainly due to a lack of high-cadence observations at high angular resolution. Understanding this type of variation could be important for our understanding of phenomena related to disk evolution. Aims . We study the morphological variability of the innermost circumstellar environment of HD 98922, focusing on its dust and gas content. Methods . Multi-epoch observations of HD 98922 at milliarcsecond resolution with VLTI/GRAVITY in the K -band at low ( R = 20) and high ( R = 4000) spectral resolution are combined with VLTI/PIONIER archival data covering a total time span of 11 yr. We interpret the interferometric visibilities and spectral energy distribution with geometrical models and through radiative transfer techniques using the code MCMax. We investigated high-spectral-resolution quantities (visibilities and differential phases) to obtain information on the properties of the HI Brackett- γ (Br γ )-line-emitting region. Results . Comparing observations taken with similar (u,v) plane coverage, we find that the squared visibilities do not vary significantly, whereas we find strong variability in the closure phases, suggesting temporal variations in the asymmetric brightness distribution associated to the disk. Our observations are best fitted by a model of a crescent-like asymmetric dust feature located at ~1 au and accounting for ~70 % of the near-infrared (NIR) emission. The feature has an almost constant magnitude and orbits the central star with a possible sub-Keplerian period of ~12 months, although a 9 month period is another, albeit less probable, solution. The radiative transfer models show that the emission originates from a small amount of carbon-rich (25%) silicates, or quantum-heated particles located in a low-density region. Among different possible scenarios, we favor hydrodynamical instabilities in the inner disk that can create a large vortex. The high spectral resolution differential phases in the Br γ line show that the hot-gas compact component is offset from the star and in some cases is located between the star and the crescent feature. The scale of the emission does not favor magnetospheric accretion as a driving mechanism. The scenario of an asymmetric disk wind or a massive accreting substellar or planetary companion is discussed. Conclusions . With this unique observational data set for HD 98922, we reveal morphological variability in the innermost 2 au of its disk region. This property is possibly common to many other protoplanetary disks, but is not commonly observed due to a lack of high-cadence observation. It is therefore important to pursue this approach with other sources for which an extended dataset with PIONIER, GRAVITY, and possibly MATISSE is available.
Related Topics
Concepts
Physics
Astrophysics
Radiative transfer
Spectral energy distribution
Young stellar object
Context (archaeology)
Brightness
Spectral resolution
Protoplanetary disk
Angular resolution (graph drawing)
Astronomy
Planet
Spectral line
Galaxy
Star formation
Quantum mechanics
Paleontology
Combinatorics
Biology
Mathematics
Metadata
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.1051/0004-6361/202346926
- OA Status
- hybrid
- Cited By
- 6
- References
- 106
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4391340288
All OpenAlex metadata
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W4391340288Canonical identifier for this work in OpenAlex
- DOI
-
https://doi.org/10.1051/0004-6361/202346926Digital Object Identifier
- Title
-
The GRAVITY young stellar object surveyWork title
- Type
-
articleOpenAlex work type
- Language
-
enPrimary language
- Publication year
-
2024Year of publication
- Publication date
-
2024-01-30Full publication date if available
- Authors
-
V. Ganci, Lucas Labadie, K. Perraut, A. Wojtczak, J. Kaufhold, M. Benisty, E. Alécian, G. Bourdarot, W. Brandner, A. Caratti o Garatti, C. Dougados, R. García López, J. Sánchez-Bermúdez, A. Soulain, A. Amorim, Jean-Philippe Berger, P. Caselli, Y. Clénet, A. Drescher, A. Eckart, F. Eisenhauer, M. Fabricius, H. Feuchtgruber, P. García, É. Gendron, R. Genzel, S. Gillessen, Sierra L. Grant, G. Heißel, Thomas Henning, M. Horrobin, L. Jocou, P. Kervella, S. Lacour, V. Lapeyrère, J.-B. Le Bouquin, Pierre Léna, D. Lutz, F. Mang, Nuno Morujão, T. Ott, T. Paumard, G. Perrin, D. Ribeiro, M. S. Bordoni, S. Scheithauer, J. Shangguan, Thomas Shimizu, C. Straubmeier, E. Sturm, L. J. Tacconi, E. F. van Dishoeck, F. Vincent, J. WoillezList of authors in order
- Landing page
-
https://doi.org/10.1051/0004-6361/202346926Publisher landing page
- Open access
-
YesWhether a free full text is available
- OA status
-
hybridOpen access status per OpenAlex
- OA URL
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https://doi.org/10.1051/0004-6361/202346926Direct OA link when available
- Concepts
-
Physics, Astrophysics, Radiative transfer, Spectral energy distribution, Young stellar object, Context (archaeology), Brightness, Spectral resolution, Protoplanetary disk, Angular resolution (graph drawing), Astronomy, Planet, Spectral line, Galaxy, Star formation, Quantum mechanics, Paleontology, Combinatorics, Biology, MathematicsTop concepts (fields/topics) attached by OpenAlex
- Cited by
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6Total citation count in OpenAlex
- Citations by year (recent)
-
2025: 3, 2024: 3Per-year citation counts (last 5 years)
- References (count)
-
106Number of works referenced by this work
- Related works (count)
-
10Other works algorithmically related by OpenAlex
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| abstract_inverted_index.time | 128 |
| abstract_inverted_index.type | 52 |
| abstract_inverted_index.vary | 195 |
| abstract_inverted_index.wind | 375 |
| abstract_inverted_index.with | 99, 121, 142, 182, 258, 440, 448 |
| abstract_inverted_index.(25%) | 292 |
| abstract_inverted_index.(NIR) | 244 |
| abstract_inverted_index.(u,v) | 184 |
| abstract_inverted_index.-band | 104 |
| abstract_inverted_index.4000) | 116 |
| abstract_inverted_index.98922 | 95 |
| abstract_inverted_index.Among | 302 |
| abstract_inverted_index.cases | 345 |
| abstract_inverted_index.could | 55 |
| abstract_inverted_index.disk. | 217 |
| abstract_inverted_index.disks | 12 |
| abstract_inverted_index.favor | 307, 362 |
| abstract_inverted_index.found | 33 |
| abstract_inverted_index.inner | 312 |
| abstract_inverted_index.large | 318 |
| abstract_inverted_index.model | 225 |
| abstract_inverted_index.month | 269 |
| abstract_inverted_index.other | 417, 441 |
| abstract_inverted_index.plane | 185 |
| abstract_inverted_index.scale | 356 |
| abstract_inverted_index.short | 28 |
| abstract_inverted_index.small | 288 |
| abstract_inverted_index.study | 70 |
| abstract_inverted_index.taken | 181 |
| abstract_inverted_index.their | 25 |
| abstract_inverted_index.total | 127 |
| abstract_inverted_index.using | 150 |
| abstract_inverted_index.which | 444 |
| abstract_inverted_index.young | 16 |
| abstract_inverted_index.98922, | 81, 396 |
| abstract_inverted_index.MCMax. | 153 |
| abstract_inverted_index.albeit | 273 |
| abstract_inverted_index.almost | 250 |
| abstract_inverted_index.amount | 289 |
| abstract_inverted_index.common | 14, 414 |
| abstract_inverted_index.create | 316 |
| abstract_inverted_index.disks, | 419 |
| abstract_inverted_index.energy | 140 |
| abstract_inverted_index.fitted | 222 |
| abstract_inverted_index.mainly | 38 |
| abstract_inverted_index.models | 144, 280 |
| abstract_inverted_index.obtain | 163 |
| abstract_inverted_index.offset | 338 |
| abstract_inverted_index.orbits | 254 |
| abstract_inverted_index.period | 262, 270 |
| abstract_inverted_index.phases | 325 |
| abstract_inverted_index.pursue | 437 |
| abstract_inverted_index.reveal | 398 |
| abstract_inverted_index.strong | 200 |
| abstract_inverted_index.toward | 22 |
| abstract_inverted_index.unique | 390 |
| abstract_inverted_index.Context | 0 |
| abstract_inverted_index.MATISSE | 453 |
| abstract_inverted_index.Methods | 89 |
| abstract_inverted_index.Results | 177 |
| abstract_inverted_index.angular | 48 |
| abstract_inverted_index.between | 348 |
| abstract_inverted_index.central | 256 |
| abstract_inverted_index.changes | 23 |
| abstract_inverted_index.closure | 204 |
| abstract_inverted_index.compact | 335 |
| abstract_inverted_index.dataset | 447 |
| abstract_inverted_index.driving | 367 |
| abstract_inverted_index.feature | 231, 247 |
| abstract_inverted_index.hot-gas | 334 |
| abstract_inverted_index.located | 232, 297, 347 |
| abstract_inverted_index.massive | 378 |
| abstract_inverted_index.months, | 265 |
| abstract_inverted_index.phases) | 161 |
| abstract_inverted_index.phases, | 205 |
| abstract_inverted_index.region. | 176, 301, 409 |
| abstract_inverted_index.related | 63 |
| abstract_inverted_index.similar | 183 |
| abstract_inverted_index.sources | 442 |
| abstract_inverted_index.squared | 191 |
| abstract_inverted_index.stellar | 17 |
| abstract_inverted_index.through | 146 |
| abstract_inverted_index.vortex. | 319 |
| abstract_inverted_index.whereas | 197 |
| abstract_inverted_index.GRAVITY, | 450 |
| abstract_inverted_index.However, | 19 |
| abstract_inverted_index.PIONIER, | 449 |
| abstract_inverted_index.Temporal | 2 |
| abstract_inverted_index.although | 266 |
| abstract_inverted_index.another, | 272 |
| abstract_inverted_index.approach | 439 |
| abstract_inverted_index.archival | 123 |
| abstract_inverted_index.combined | 120 |
| abstract_inverted_index.commonly | 423 |
| abstract_inverted_index.constant | 251 |
| abstract_inverted_index.content. | 88 |
| abstract_inverted_index.covering | 125 |
| abstract_inverted_index.crescent | 353 |
| abstract_inverted_index.emission | 284, 359 |
| abstract_inverted_index.evidence | 20 |
| abstract_inverted_index.extended | 446 |
| abstract_inverted_index.feature. | 354 |
| abstract_inverted_index.focusing | 82 |
| abstract_inverted_index.objects. | 18 |
| abstract_inverted_index.observed | 424 |
| abstract_inverted_index.pointing | 21 |
| abstract_inverted_index.possible | 260, 304 |
| abstract_inverted_index.possibly | 413, 452 |
| abstract_inverted_index.property | 411 |
| abstract_inverted_index.scenario | 370 |
| abstract_inverted_index.sources, | 37 |
| abstract_inverted_index.spectral | 117, 139, 322 |
| abstract_inverted_index.temporal | 207 |
| abstract_inverted_index.transfer | 148, 279 |
| abstract_inverted_index.Brackett- | 171 |
| abstract_inverted_index.Comparing | 179 |
| abstract_inverted_index.accreting | 379 |
| abstract_inverted_index.accretion | 364 |
| abstract_inverted_index.companion | 383 |
| abstract_inverted_index.component | 336 |
| abstract_inverted_index.coverage, | 186 |
| abstract_inverted_index.different | 303 |
| abstract_inverted_index.emission. | 245 |
| abstract_inverted_index.important | 57, 435 |
| abstract_inverted_index.innermost | 76, 403 |
| abstract_inverted_index.interpret | 134 |
| abstract_inverted_index.magnitude | 252 |
| abstract_inverted_index.particles | 296 |
| abstract_inverted_index.phenomena | 62 |
| abstract_inverted_index.planetary | 382 |
| abstract_inverted_index.probable, | 275 |
| abstract_inverted_index.radiative | 147, 278 |
| abstract_inverted_index.solution. | 276 |
| abstract_inverted_index.therefore | 434 |
| abstract_inverted_index.variation | 54 |
| abstract_inverted_index.accounting | 237 |
| abstract_inverted_index.associated | 214 |
| abstract_inverted_index.asymmetric | 211, 229, 373 |
| abstract_inverted_index.available. | 455 |
| abstract_inverted_index.brightness | 212 |
| abstract_inverted_index.discussed. | 385 |
| abstract_inverted_index.evolution. | 66 |
| abstract_inverted_index.mechanism. | 368 |
| abstract_inverted_index.morphology | 26 |
| abstract_inverted_index.originates | 285 |
| abstract_inverted_index.properties | 9, 167 |
| abstract_inverted_index.quantities | 157 |
| abstract_inverted_index.resolution | 98, 118, 323 |
| abstract_inverted_index.scenarios, | 305 |
| abstract_inverted_index.silicates, | 293 |
| abstract_inverted_index.substellar | 380 |
| abstract_inverted_index.suggesting | 206 |
| abstract_inverted_index.techniques | 149 |
| abstract_inverted_index.timescales | 29 |
| abstract_inverted_index.variations | 208 |
| abstract_inverted_index.Conclusions | 386 |
| abstract_inverted_index.Multi-epoch | 91 |
| abstract_inverted_index.carbon-rich | 291 |
| abstract_inverted_index.environment | 78 |
| abstract_inverted_index.geometrical | 143 |
| abstract_inverted_index.information | 164 |
| abstract_inverted_index.low-density | 300 |
| abstract_inverted_index.photometric | 6 |
| abstract_inverted_index.resolution. | 49 |
| abstract_inverted_index.variability | 3, 73, 201, 400 |
| abstract_inverted_index.VLTI/GRAVITY | 100 |
| abstract_inverted_index.VLTI/PIONIER | 122 |
| abstract_inverted_index.differential | 160, 324 |
| abstract_inverted_index.distribution | 141, 213 |
| abstract_inverted_index.high-cadence | 44, 430 |
| abstract_inverted_index.investigated | 155 |
| abstract_inverted_index.observation. | 431 |
| abstract_inverted_index.observations | 45, 92, 180, 219 |
| abstract_inverted_index.visibilities | 137, 192 |
| abstract_inverted_index.(visibilities | 158 |
| abstract_inverted_index.Understanding | 50 |
| abstract_inverted_index.circumstellar | 77 |
| abstract_inverted_index.crescent-like | 228 |
| abstract_inverted_index.instabilities | 309 |
| abstract_inverted_index.morphological | 72, 399 |
| abstract_inverted_index.near-infrared | 243 |
| abstract_inverted_index.observational | 391 |
| abstract_inverted_index.spectroscopic | 8 |
| abstract_inverted_index.sub-Keplerian | 261 |
| abstract_inverted_index.understanding | 60 |
| abstract_inverted_index.hydrodynamical | 308 |
| abstract_inverted_index.magnetospheric | 363 |
| abstract_inverted_index.milliarcsecond | 97 |
| abstract_inverted_index.protoplanetary | 11, 418 |
| abstract_inverted_index.quantum-heated | 295 |
| abstract_inverted_index.significantly, | 196 |
| abstract_inverted_index.)-line-emitting | 175 |
| abstract_inverted_index.interferometric | 136 |
| abstract_inverted_index.high-spectral-resolution | 156 |
| cited_by_percentile_year.max | 97 |
| cited_by_percentile_year.min | 96 |
| countries_distinct_count | 6 |
| institutions_distinct_count | 54 |
| sustainable_development_goals[0].id | https://metadata.un.org/sdg/7 |
| sustainable_development_goals[0].score | 0.6700000166893005 |
| sustainable_development_goals[0].display_name | Affordable and clean energy |
| citation_normalized_percentile.value | 0.88540321 |
| citation_normalized_percentile.is_in_top_1_percent | False |
| citation_normalized_percentile.is_in_top_10_percent | True |