The DOI matches its Crossref record; 4 of the 4 references it cites were found in a registry or an index.
The minimum-mass extrasolar nebula: in situ formation of close-in super-Earths
Open accessAbstract
Close-in super-Earths, with radii R ≈ 2–5R⊕ and orbital periods P < 100 d, orbit more than half, and perhaps nearly all, Sun-like stars in the Universe. We use this omnipresent population to construct the minimum-mass extrasolar nebula (MMEN), the circumstellar disc of solar-composition solids and gas from which such planets formed, if they formed near their current locations and did not migrate. In a series of back-of-the-envelope calculations, we demonstrate how in situ formation in the MMEN is fast, efficient, and can reproduce many of the observed properties of close-in super-Earths, including their gas-to-rock fractions. Testable predictions are discussed.
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Cites
Galactic Dynamics: Second Edition
Binney, J., & Tremaine, S. (2008) · doi:10.1515/9781400828722 · Cited by 4,375 · cited 1×
“(8) The Toomre stability parameter (e.g., Binney & Tremaine 2008) for our gas disk is Qgas = cgasΩ πGσgas = 15F −1disk ( a 0.2 AU )0.1 , (9) large enough compared to unity that the MMEN is gravitationally stable.”
InfluentialA super-Earth transiting a nearby low-mass star
Charbonneau, D., Berta, Z. K., Irwin, J., Burke, C. J., Nutzman, P., Buchhave, L. A., Lovis, C., Bonfils, X., Latham, D. W., Udry, S., et al. (2009) · Nature · doi:10.1038/nature08679 · Cited by 797
The Occurrence and Mass Distribution of Close-in Super-Earths, Neptunes, and Jupiters
Howard, A. W., Marcy, G. W., Johnson, J. A., Fischer, D. A., Wright, J. T., Isaacson, H., Valenti, J. A., Anderson, J., Lin, D. N. C., & Ida, S. (2010) · Science · doi:10.1126/science.1194854 · Cited by 635
SECULAR CHAOS AND THE PRODUCTION OF HOT JUPITERS
Wu, Y., & Lithwick, Y. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/735/2/109 · Cited by 432
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Gillon, M., Triaud, A. H. M. J., Demory, B.-O., Jehin, E., Agol, E., Deck, K. M., Lederer, S. M., de Wit, J., Burdanov, A., Ingalls, J. G., et al. (2017) · Nature · doi:10.1038/nature21360 · Cited by 1,555
The California-Kepler Survey. III. A Gap in the Radius Distribution of Small Planets*
Fulton, B. J., Petigura, E. A., Howard, A. W., Isaacson, H., Marcy, G. W., Cargile, P. A., Hebb, L., Weiss, L. M., Johnson, J. A., Morton, T. D., et al. (2017) · The Astronomical Journal · doi:10.3847/1538-3881/aa80eb · Cited by 1,446
The Occurrence and Architecture of Exoplanetary Systems
Winn, J. N., & Fabrycky, D. C. (2015) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-082214-122246 · Cited by 891
UNDERSTANDING THE MASS-RADIUS RELATION FOR SUB-NEPTUNES: RADIUS AS A PROXY FOR COMPOSITION
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Dawson, R. I., & Johnson, J. A. (2018) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081817-051853 · Cited by 622
Metadata
- Authors
- Chiang, E., & Laughlin, G.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2013-04-11
- Volume
- 431
- Issue
- 4
- Pages
- 3444-3455
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2096258061
- Cited by
- 460
- References
- 4
- FWCI
- 28.62
- Type
- journal article
- Language
- en
- Open access
- green
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- Chiang, E., & Laughlin, G. (2013). The minimum-mass extrasolar nebula: in situ formation of close-in super-Earths. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1093/mnras/stt424
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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