The DOI matches its Crossref record; 51 of the 51 references it cites were found in a registry or an index.
RINGED SUBSTRUCTURE AND A GAP AT 1 au IN THE NEAREST PROTOPLANETARY DISK
Open accessAbstract
We present long baseline Atacama Large Millimeter/submillimeter Array (ALMA) observations of the 870 μ m continuum emission from the nearest gas-rich protoplanetary disk, around TW Hya, that trace millimeter-sized particles down to spatial scales as small as 1 au (20 mas). These data reveal a series of concentric ring-shaped substructures in the form of bright zones and narrow dark annuli (1–6 au) with modest contrasts (5%–30%). We associate these features with concentrations of solids that have had their inward radial drift slowed or stopped, presumably at local gas pressure maxima. No significant non-axisymmetric structures are detected. Some of the observed features occur near temperatures that may be associated with the condensation fronts of major volatile species, but the relatively small brightness contrasts may also be a consequence of magnetized disk evolution (the so-called zonal flows). Other features, particularly a narrow dark annulus located only 1 au from the star, could indicate interactions between the disk and young planets. These data signal that ordered substructures on ∼au scales can be common, fundamental factors in disk evolution and that high-resolution microwave imaging can help characterize them during the epoch of planet formation.
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
Astropy: A community Python package for astronomy
The Astropy Collaboration, Robitaille, T. P., Tollerud, E. J., Greenfield, P., Droettboom, M., Bray, E., Aldcroft, T., Davis, M., Ginsburg, A., Price-Whelan, A. M., et al. (2013) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201322068 · Cited by 14,620
Balbus, S. A., & Hawley, J. F. (1991) · The Astrophysical Journal · doi:10.1086/170270 · Cited by 4,469
Validation of the new Hipparcos reduction
van Leeuwen, F. (2007) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20078357 · Cited by 3,736
Aerodynamics of solid bodies in the solar nebula
Weidenschilling, S. J. (1977) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/180.2.57 · Cited by 1,984
Protoplanetary Disks and Their Evolution
Williams, J. P., & Cieza, L. A. (2011) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081710-102548 · Cited by 1,403
Astrophysics Source Code Library
Allen, A., DuPrie, K., Berriman, G. B., Hanisch, R. J., Mink, J. D., & Teuben, P. J. (2012) · arXiv (Cornell University) · doi:10.48550/arxiv.1212.1916 · Cited by 1,228
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-citationLin, D. N. C., & Papaloizou, J. (1986) · The Astrophysical Journal · doi:10.1086/164653 · Cited by 1,054
Rapid growth of gas-giant cores by pebble accretion
Lambrechts, M., & Johansen, A. (2012) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201219127 · Cited by 875
Planet-Disk Interaction and Orbital Evolution
Kley, W., & Nelson, R. P. (2012) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081811-125523 · Cited by 722
Cited by
Phantom: A Smoothed Particle Hydrodynamics and Magnetohydrodynamics Code for Astrophysics
Price, D. J., Wurster, J., Tricco, T. S., Nixon, C., Toupin, S., Pettitt, A., Chan, C., Mentiplay, D., Laibe, G., Glover, S., et al. (2018) · Publications of the Astronomical Society of Australia · doi:10.1017/pasa.2018.25 · Cited by 429
Molecules with ALMA at Planet-forming Scales (MAPS). I. Program Overview and Highlights
Öberg, K. I., Guzmán, V. V., Walsh, C., Aikawa, Y., Bergin, E. A., Law, C. J., Loomis, R. A., Alarcón, F., Andrews, S. M., Bae, J., et al. (2021) · The Astrophysical Journal Supplement Series · doi:10.3847/1538-4365/ac1432 · Cited by 280
Self-citationConstraining the Time Interval for the Origin of Life on Earth
Pearce, B. K. D., Tupper, A. S., Pudritz, R. E., & Higgs, P. G. (2018) · Astrobiology · doi:10.1089/ast.2017.1674 · Cited by 140
Giant planet formation in radially structured protoplanetary discs
Coleman, G. A. L., & Nelson, R. P. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw1177 · Cited by 79
Metadata
- Authors
- Andrews, S. M., Wilner, D. J., Zhu, Z., Birnstiel, T., Carpenter, J. M., Pérez, L. M., Bai, X.-N., Öberg, K. I., Hughes, A. M., Isella, A., & Ricci, L.
- Venue
- The Astrophysical Journal Letters
- Publisher
- American Astronomical Society
- Published
- 2016-03-31
- Volume
- 820
- Issue
- 2
- Pages
- L40
- ISSN
- 2041-8205 (ISSN-L)
- 2041-8213
- OpenAlex
- W2314445977
- Cited by
- 561
- References
- 51
- FWCI
- 53.39
- 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: RINGED SUBSTRUCTURE AND A GAP AT 1 au IN THE NEAREST PROTOPLANETARY DISK. https://app.cochat.ai/papers/10.3847/2041-8205/820/2/l40
- The paper
- Andrews, S. M., Wilner, D. J., Zhu, Z., Birnstiel, T., Carpenter, J. M., Pérez, L. M., Bai, X.-N., Öberg, K. I., Hughes, A. M., Isella, A., & Ricci, L. (2016). RINGED SUBSTRUCTURE AND A GAP AT 1 au IN THE NEAREST PROTOPLANETARY DISK. The Astrophysical Journal Letters. https://doi.org/10.3847/2041-8205/820/2/l40
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.