The DOI matches its Crossref record; 59 of the 59 references it cites were found in a registry or an index.
The Disk Substructures at High Angular Resolution Project (DSHARP). VI. Dust Trapping in Thin-ringed Protoplanetary Disks
Open accessAbstract
A large fraction of the protoplanetary disks observed with ALMA display multiple well-defined and nearly perfectly circular rings in the continuum, in many cases with substantial peak-to-valley contrast. The DSHARP campaign shows that several of these rings are very narrow in radial extent. In this Letter we test the hypothesis that these dust rings are caused by dust trapping in radial pressure bumps, and if confirmed, put constraints on the physics of the dust trapping mechanism. We model this process analytically in 1D, assuming axisymmetry. By comparing this model to the data, we find that all rings are consistent with dust trapping. Based on a plausible model of the dust temperature we find that several rings are narrower than the pressure scale height, providing strong evidence for dust trapping. The rings have peak absorption optical depth in the range between 0.2 and 0.5. The dust masses stored in each of these rings is of the order of tens of Earth masses, though much ambiguity remains due to the uncertainty of the dust opacities. The dust rings are dense enough to potentially trigger the streaming instability, but our analysis cannot give proof of this mechanism actually operating. Our results show, however, that the combination of very low and very large grains can be excluded by the data for all the rings studied in this Letter.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
<tt>emcee</tt>: The MCMC Hammer
Foreman-Mackey, D., Hogg, D. W., Lang, D., & Goodman, J. (2013) · Publications of the Astronomical Society of the Pacific · doi:10.1086/670067 · Cited by 12,414
The Evolution of Viscous Discs and the Origin of the Nebular Variables
Lynden-Bell, D., & Pringle, J. E. (1974) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/168.3.603 · Cited by 2,668
Spectral Energy Distributions of T Tauri Stars with Passive Circumstellar Disks
Chiang, E. I., & Goldreich, P. (1997) · The Astrophysical Journal · doi:10.1086/304869 · Cited by 1,683
Accretion and the Evolution of T Tauri Disks
Hartmann, L., Calvet, N., Gullbring, E., & D'Alessio, P. (1998) · The Astrophysical Journal · doi:10.1086/305277 · Cited by 1,569
Rapid planetesimal formation in turbulent circumstellar disks
Johansen, A., Oishi, J. S., Low, M.-M. M., Klahr, H., Henning, T., & Youdin, A. (2007) · Nature · doi:10.1038/nature06086 · Cited by 1,241
Streaming Instabilities in Protoplanetary Disks
Youdin, A. N., & Goodman, J. (2005) · The Astrophysical Journal · doi:10.1086/426895 · Cited by 1,198
Partnership, A., Brogan, C. L., Pérez, L. M., Hunter, T. R., Dent, W. R. F., Hales, A. S., Hills, R. E., Corder, S., Fomalont, E. B., Vlahakis, C., et al. (2015) · The Astrophysical Journal · doi:10.1088/2041-8205/808/1/l3 · Cited by 1,174
Self-citationAndrews, S. M., Huang, J., Pérez, L. M., Isella, A., Dullemond, C. P., Kurtovic, N. T., Guzmán, V. V., Carpenter, J. M., Wilner, D. J., Zhang, S., et al. (2018) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/aaf741 · Cited by 1,128
Self-citationPassive Irradiated Circumstellar Disks with an Inner Hole
Dullemond, C. P., Dominik, C., & Natta, A. (2001) · The Astrophysical Journal · doi:10.1086/323057 · Cited by 797
Self-citationThe Gas Drag Effect on the Elliptic Motion of a Solid Body in the Primordial Solar Nebula
Adachi, I., Hayashi, C., & Nakazawa, K. (1976) · Progress of Theoretical Physics · doi:10.1143/ptp.56.1756 · Cited by 726
Cited by
Zhang, S., Zhu, Z., Huang, J., Guzmán, V. V., Andrews, S. M., Birnstiel, T., Dullemond, C. P., Carpenter, J. M., Isella, A., Pérez, L. M., et al. (2018) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/aaf744 · Cited by 389
Self-citation
Metadata
- Authors
- Dullemond, C. P., Birnstiel, T., Huang, J., Kurtovic, N. T., Andrews, S. M., Guzmán, V. V., Pérez, L. M., Isella, A., Zhu, Z., Benisty, M., Wilner, D. J., Bai, X.-N., Carpenter, J. M., Zhang, S., & Ricci, L.
- Venue
- The Astrophysical Journal Letters
- Publisher
- American Astronomical Society
- Published
- 2018-12-20
- Volume
- 869
- Issue
- 2
- Pages
- L46
- ISSN
- 2041-8205 (ISSN-L)
- 2041-8213
- OpenAlex
- W2904278424
- Cited by
- 391
- References
- 59
- FWCI
- 20.08
- Type
- journal article
- Language
- en
- Open access
- bronze
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: The Disk Substructures at High Angular Resolution Project (DSHARP). VI. Dust Trapping in Thin-ringed Protoplanetary Disks. https://app.cochat.ai/papers/10.3847/2041-8213/aaf742
- The paper
- Dullemond, C. P., Birnstiel, T., Huang, J., Kurtovic, N. T., Andrews, S. M., Guzmán, V. V., Pérez, L. M., Isella, A., Zhu, Z., Benisty, M., Wilner, D. J., Bai, X.-N., Carpenter, J. M., Zhang, S., & Ricci, L. (2018). The Disk Substructures at High Angular Resolution Project (DSHARP). VI. Dust Trapping in Thin-ringed Protoplanetary Disks. The Astrophysical Journal Letters. https://doi.org/10.3847/2041-8213/aaf742
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.
