Gap Opening and Inner Disk Structure in the Strongly Accreting Transition Disk of DM Tau Article Swipe
Logan Francis
,
Nienke van der Marel
,
Doug Johnstone
,
Eiji Akiyama
,
Simon Bruderer
,
Ruobing Dong
,
Jun Hashimoto
,
Hauyu Baobab Liu
,
Takayuki Muto
,
Yi Yang
·
YOU?
·
· 2022
· Open Access
·
· DOI: https://doi.org/10.3847/1538-3881/ac7ffb
YOU?
·
· 2022
· Open Access
·
· DOI: https://doi.org/10.3847/1538-3881/ac7ffb
Large inner dust gaps in transition disks are frequently posited as evidence of giant planets sculpting gas and dust in the disk, or the opening of a gap by photoevaporative winds. Although the former hypothesis is strongly supported by the observations of planets and deep depletions in gas within the gap in some disks, many T Tauri stars hosting transition disks accrete at rates typical for an undepleted disk, raising the question of how gap opening occurs in these objects. We thus present an analysis of the structure of the transition disk around the T Tauri star DM Tau, which is strongly accreting (∼10 −8.3 M ⊙ yr −1 ) and turbulent ( α = 0.078 ± 0.02). Using the Dust And LInes thermochemical code, we fit disk models to simultaneously reproduce the accretion rate, high level of turbulence, the gas traced by ALMA Band 6 observations of 12 CO, 13 CO, and C 18 O J = 2–1 lines, and the observed dust emission from the millimeter continuum and spectral energy distribution. We find a shallow depletion in gas surface density of ∼10 relative to the outer disk and a gas-rich inner disk that is consistent with the observations. The planet mass of <1 M Jup implied by the gap depth is in tension with predictions for dust trapping in a highly viscous disk, which requires a more massive planet of ∼10 M Jup . Photoevaporative models including a dead zone can qualitatively reproduce some features of the DM Tau disk, but still struggle to explain the high accretion rates and the observed millimeter-continuum flux.
Related Topics
Concepts
Physics
Astrophysics
Planet
T Tauri star
Protoplanetary disk
Submillimeter Array
Accretion (finance)
Spectral energy distribution
Stars
Protoplanet
Astronomy
Millimeter
Turbulence
Thick disk
Star formation
Galaxy
Thermodynamics
Halo
Metadata
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.3847/1538-3881/ac7ffb
- https://iopscience.iop.org/article/10.3847/1538-3881/ac7ffb/pdf
- OA Status
- gold
- Cited By
- 11
- References
- 97
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4292493815
All OpenAlex metadata
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W4292493815Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.3847/1538-3881/ac7ffbDigital Object Identifier
- Title
-
Gap Opening and Inner Disk Structure in the Strongly Accreting Transition Disk of DM TauWork title
- Type
-
articleOpenAlex work type
- Language
-
enPrimary language
- Publication year
-
2022Year of publication
- Publication date
-
2022-08-19Full publication date if available
- Authors
-
Logan Francis, Nienke van der Marel, Doug Johnstone, Eiji Akiyama, Simon Bruderer, Ruobing Dong, Jun Hashimoto, Hauyu Baobab Liu, Takayuki Muto, Yi YangList of authors in order
- Landing page
-
https://doi.org/10.3847/1538-3881/ac7ffbPublisher landing page
- PDF URL
-
https://iopscience.iop.org/article/10.3847/1538-3881/ac7ffb/pdfDirect link to full text PDF
- Open access
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YesWhether a free full text is available
- OA status
-
goldOpen access status per OpenAlex
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https://iopscience.iop.org/article/10.3847/1538-3881/ac7ffb/pdfDirect OA link when available
- Concepts
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Physics, Astrophysics, Planet, T Tauri star, Protoplanetary disk, Submillimeter Array, Accretion (finance), Spectral energy distribution, Stars, Protoplanet, Astronomy, Millimeter, Turbulence, Thick disk, Star formation, Galaxy, Thermodynamics, HaloTop concepts (fields/topics) attached by OpenAlex
- Cited by
-
11Total citation count in OpenAlex
- Citations by year (recent)
-
2025: 2, 2024: 4, 2023: 4, 2022: 1Per-year citation counts (last 5 years)
- References (count)
-
97Number of works referenced by this work
- Related works (count)
-
10Other works algorithmically related by OpenAlex
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| abstract_inverted_index.Using | 119 |
| abstract_inverted_index.code, | 125 |
| abstract_inverted_index.depth | 212 |
| abstract_inverted_index.disk, | 22, 69, 225, 252 |
| abstract_inverted_index.disks | 7, 61 |
| abstract_inverted_index.flux. | 266 |
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| abstract_inverted_index.level | 137 |
| abstract_inverted_index.outer | 188 |
| abstract_inverted_index.rate, | 135 |
| abstract_inverted_index.rates | 64, 261 |
| abstract_inverted_index.stars | 58 |
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| abstract_inverted_index.these | 79 |
| abstract_inverted_index.which | 100, 226 |
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| abstract_inverted_index.(∼10 | 104 |
| abstract_inverted_index.0.02). | 118 |
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| abstract_inverted_index.highly | 223 |
| abstract_inverted_index.lines, | 160 |
| abstract_inverted_index.models | 129, 238 |
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| abstract_inverted_index.planet | 202, 231 |
| abstract_inverted_index.traced | 142 |
| abstract_inverted_index.winds. | 31 |
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| abstract_inverted_index.accrete | 62 |
| abstract_inverted_index.density | 182 |
| abstract_inverted_index.explain | 257 |
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| abstract_inverted_index.implied | 208 |
| abstract_inverted_index.massive | 230 |
| abstract_inverted_index.opening | 25, 76 |
| abstract_inverted_index.planets | 15, 43 |
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| abstract_inverted_index.surface | 181 |
| abstract_inverted_index.tension | 215 |
| abstract_inverted_index.typical | 65 |
| abstract_inverted_index.viscous | 224 |
| abstract_inverted_index.Abstract | 0 |
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| abstract_inverted_index.analysis | 85 |
| abstract_inverted_index.emission | 165 |
| abstract_inverted_index.evidence | 12 |
| abstract_inverted_index.features | 247 |
| abstract_inverted_index.gas-rich | 192 |
| abstract_inverted_index.objects. | 80 |
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| abstract_inverted_index.question | 72 |
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| abstract_inverted_index.accreting | 103 |
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| abstract_inverted_index.depletion | 178 |
| abstract_inverted_index.including | 239 |
| abstract_inverted_index.reproduce | 132, 245 |
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| abstract_inverted_index.structure | 88 |
| abstract_inverted_index.supported | 38 |
| abstract_inverted_index.turbulent | 112 |
| abstract_inverted_index.consistent | 197 |
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| abstract_inverted_index.hypothesis | 35 |
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| abstract_inverted_index.transition | 6, 60, 91 |
| abstract_inverted_index.undepleted | 68 |
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| abstract_inverted_index.turbulence, | 139 |
| abstract_inverted_index.observations | 41, 147 |
| abstract_inverted_index.distribution. | 173 |
| abstract_inverted_index.observations. | 200 |
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| abstract_inverted_index.thermochemical | 124 |
| abstract_inverted_index.Photoevaporative | 237 |
| abstract_inverted_index.photoevaporative | 30 |
| abstract_inverted_index.millimeter-continuum | 265 |
| cited_by_percentile_year.max | 98 |
| cited_by_percentile_year.min | 89 |
| corresponding_author_ids | https://openalex.org/A5015822543 |
| countries_distinct_count | 5 |
| institutions_distinct_count | 10 |
| corresponding_institution_ids | https://openalex.org/I212119943 |
| sustainable_development_goals[0].id | https://metadata.un.org/sdg/7 |
| sustainable_development_goals[0].score | 0.49000000953674316 |
| sustainable_development_goals[0].display_name | Affordable and clean energy |
| citation_normalized_percentile.value | 0.86122473 |
| citation_normalized_percentile.is_in_top_1_percent | False |
| citation_normalized_percentile.is_in_top_10_percent | True |