The DOI matches its Crossref record; 34 of the 34 references it cites were found in a registry or an index.
On planet formation in HL Tau
Open accessAbstract
We explain the axisymmetric gaps seen in recent long-baseline observations of the HL Tau protoplanetary disc with the Atacama Large Millimetre/Submillimetre Array (ALMA) as being due to the different response of gas and dust to embedded planets in protoplanetary discs. We perform global, three-dimensional dusty smoothed particle hydrodynamics calculations of multiple planets embedded in dust/gas discs which successfully reproduce most of the structures seen in the ALMA image. We find a best match to the observations using three embedded planets with masses of 0.2, 0.27 and 0.55 MJ in the three main gaps observed by ALMA, though there remain uncertainties in the exact planet masses from the disc model.
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Cites
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
Goldreich, P., & Tremaine, S. (1980) · The Astrophysical Journal · doi:10.1086/158356 · Cited by 1,645
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
Modelling accretion in protobinary systems
Bate, M. R., Bonnell, I. A., & Price, N. M. (1995) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/277.2.362 · Cited by 910
Robitaille, T. P., Whitney, B. A., Indebetouw, R., & Wood, K. (2007) · The Astrophysical Journal Supplement Series · doi:10.1086/512039 · Cited by 869
Smoothed particle hydrodynamics and magnetohydrodynamics
Price, D. J. (2012) · Journal of Computational Physics · doi:10.1016/j.jcp.2010.12.011 · Cited by 720
Self-citationOn the width and shape of gaps in protoplanetary disks
Crida, A., Morbidelli, A., & Masset, F. (2006) · Icarus · doi:10.1016/j.icarus.2005.10.007 · Cited by 610
On the Submillimeter Opacity of Protoplanetary Disks
Draine, B. T. (2006) · The Astrophysical Journal · doi:10.1086/498130 · Cited by 501
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
Self-citationMass Constraint for a Planet in a Protoplanetary Disk from the gap Width
Kanagawa, K. D., Muto, T., Tanaka, H., Tanigawa, T., Takeuchi, T., Tsukagoshi, T., & Momose, M. (2016) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/psw037 · Cited by 150
Metadata
- Authors
- Dipierro, G., Price, D., Laibe, G., Hirsh, K., Cerioli, A., & Lodato, G.
- Venue
- Monthly Notices of the Royal Astronomical Society: Letters
- Publisher
- Oxford University Press (OUP)
- Published
- 2015-08-25
- Volume
- 453
- Issue
- 1
- Pages
- L73-L77
- ISSN
- 1745-3925 (ISSN-L)
- 1745-3933
- OpenAlex
- W1609435114
- Cited by
- 276
- References
- 34
- FWCI
- 19.68
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Dipierro, G., Price, D., Laibe, G., Hirsh, K., Cerioli, A., & Lodato, G. (2015). On planet formation in HL Tau. Monthly Notices of the Royal Astronomical Society: Letters. https://doi.org/10.1093/mnrasl/slv105
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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.
