The DOI matches its Crossref record; 52 of the 52 references it cites were found in a registry or an index.
Models of giant planet formation with migration and disc evolution
Open accessAbstract
We present a new model of giant planet formation that extends the core-accretion model of Pollack et al. (1996, Icarus, 124, 62) to include migration, disc evolution and gap formation. We show that taking these effects into account can lead to much more rapid formation of giant planets, making it compatible with the typical disc lifetimes inferred from observations of young circumstellar discs. This speed up is due to the fact that migration prevents the severe depletion of the feeding zone as observed in in situ calculations. Hence, the growing planet is never isolated and it can reach cross-over mass on a much shorter timescale. To illustrate the range of planets that can form in our model, we describe a set of simulations in which we have varied some of the initial parameters and compare the final masses and semi-major axes with those inferred from observed extra-solar planets.
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.
Claims other papers make about this one
Each is checked against this paper’s own text: does it say what the citing paper says it does?
The source backs part of the claim, not all of it — or backs it for a different population, condition or comparison.
In the citing paper
“A hot Jupiter that underwent disk migration may have an intermediate composition if it accreted gas along the way (e.g., Alibert et al. 2005).”
From Origins of Hot Jupiters (2018) · cites this paper as Alibert et al. 2005
Experimental — accuracy not yet measured
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
A Jupiter-mass companion to a solar-type star
Mayor, M., & Queloz, D. (1995) · Nature · doi:10.1038/378355a0 · Cited by 4,111
Formation of the Giant Planets by Concurrent Accretion of Solids and Gas
Pollack, J. B., Hubickyj, O., Bodenheimer, P. H., Lissauer, J. J., Podolak, M., & Greenzweig, Y. (1996) · Icarus · doi:10.1006/icar.1996.0190 · Cited by 3,152
The Evolution of Viscous Discs and the Origin of the Nebular Variables
Donald Lynden-bell, A., & Pringle, J. E. (1974) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/168.3.603 · Cited by 2,603
Disk frequencies and lifetimes in Young clusters
Haisch, Jr., Lada, E. A., & Lada, C. J. (2001) · The Astrophysical Journal · doi:10.1086/320685 · Cited by 1,723
Accretion and the Evolution of T Tauri Disks
Hartmann, L. W., Calvet, N., Gullbring, E., & D’Alessio, P. (1998) · The Astrophysical Journal · doi:10.1086/305277 · Cited by 1,560
Orbital migration of the planetary companion of 51 Pegasi to its present location
Lin, D. N. C., Bodenheimer, P., & Richardson, D. C. (1996) · Nature · doi:10.1038/380606a0 · Cited by 1,235
Low-temperature Rosseland opacities
Alexander, D. R., & Ferguson, J. W. (1994) · The Astrophysical Journal · doi:10.1086/175039 · Cited by 1,161
Disk Frequencies and Lifetimes in Young Clusters
Haisch, K. E., & Lada, C. J. (2001) · CERN Document Server (European Organization for Nuclear Research) · Cited by 1,074
Lin, D. N. C., & Papaloizou, J. (1986) · The Astrophysical Journal · doi:10.1086/164653 · Cited by 1,054
Tanaka, H., Takeuchi, T., & Ward, W. R. (2002) · The Astrophysical Journal · doi:10.1086/324713 · Cited by 1,041
Research works printed but not linked: 7
- Boss, 2002, ApJ, 566, 472
- Guillot, T., Stevenson, D. J., Hubbard, W. B., & Saumon, D. 2004, in Jupiter, ed. F. Bagenal, T. E. Dowling, W. B. McKinnon, in press
- Landau, L. D., & Lifshitz, E. M. 1959, Course of theoretical physics, Fluid Mechanics, third edition (London: Pergamon Press)
- Press, W. H., Flannery, B. P., Teukolsky, S. A., & Vetterling, W. T. 1992, Numerical Recipes: The Art of Scientific Computing, third edition (Cambridge: Cambridge Univ. Press)
- Shakura, 1973, A&A, 24, 337
- Sharp, 1984, Physica, 12D, 3
- Sibulkin, 1952, J. Aeronaut. Sci., 19, 570
Cited by
Sorted by citations
Items 301–400 of 675
Solar System Physics for Exoplanet Research
Horner, J., Kane, S. R., Marshall, J. P., Dalba, P. A., Holt, T. R., Wood, J., Maynard-Casely, H. E., Wittenmyer, R. A., Lykawka, P. S., Hill, M. L., et al. (2020) · Cited by 42
France, K., Yang, H., & Linsky, J. L. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/729/1/7 · Cited by 43
Habitable Zones in the Universe
González, G. (2005) · CERN Document Server (European Organization for Nuclear Research) · Cited by 43
Monte-Carlo simulation of Callisto’s exosphere
Vorburger, A., Wurz, P., Lammer, H., Barabash, S., & Mousis, O. J. (2015) · Icarus · doi:10.1016/j.icarus.2015.07.035 · Cited by 42
Characterization of exoplanets from their formation III: The statistics of planetary luminosities
Mordasini, C., Mollière, P., & Marleau, G.-D. (2017) · BORIS (University Library Bern) · doi:10.7892/boris.112379 · Cited by 42
Self-citationAn alternative origin for debris rings of planetesimals
Nayakshin, S., & Cha, S. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21003.x · Cited by 41
Accretion disks around Jupiter and Saturn at the stage of regular satellite formation
Макалкин, А. Б., & Дорофеева, В. А. (2014) · Solar System Research · doi:10.1134/s0038094614010067 · Cited by 41
Microlensing events indicate that super-Earth exoplanets are common in Jupiter-like orbits.
Zang, W., Jung, Y., Yee, J., Hwang, K., Yang, H.-J., Udalski, A., Sumi, T., Gould, A., Mao, S., Albrow, M., et al. (2025) · Science · doi:10.1126/science.adn6088 · Cited by 37
Composition of Ices in Low‐Mass Extrasolar Planets
Marboeuf, U., Mousis, O. J., Ehrenreich, D., Alibert, Y., Cassan, A., Wakelam, V., & Beaulieu, J. (2008) · The Astrophysical Journal · doi:10.1086/588777 · Cited by 41
Self-citationWard-Duong, K., Patience, J., Bulger, J., van der Plas, G., Ménard, F., Pinte, C., Jackson, A. P., Bryden, G., Turner, N. J., Harvey, P. M., et al. (2018) · The Astronomical Journal · doi:10.3847/1538-3881/aaa128 · Cited by 44
The reliability of approximate radiation transport methods for irradiated disk studies
Kuiper, R., & Klessen, R. S. (2013) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201321404 · Cited by 40
Trapping of giant-planet cores – I. Vortex aided trapping at the outer dead zone edge
Regály, Z., Sándor, Z., Csomós, P., & Ataiee, S. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt936 · Cited by 40
Leconte, J., Baraffe, I., Chabrier, G., Barman, T., & Levrard, B. (2009) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200911896 · Cited by 42
The Origin of the Natural Satellites
Peale, S. J., & Canup, R. M. (2015) · Elsevier eBooks · doi:10.1016/b978-0-444-53802-4.00177-9 · Cited by 42
MIGRATION AND GROWTH OF PROTOPLANETARY EMBRYOS. I. CONVERGENCE OF EMBRYOS IN PROTOPLANETARY DISKS
Zhang, X., Liu, B., Lin, D. N. C., & Li, H. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/797/1/20 · Cited by 39
PRECISION RADIAL VELOCITIES WITH CSHELL
Crockett, C., Mahmud, N., Prato, L., Johns-Krull, C., Jaffe, D., & Beichman, C. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/735/2/78 · Cited by 18
Cosmochemical consequences of particle trajectories during FU Orionis outbursts by the early Sun
Boss, A., Alexander, C. M. O. '., & Podolak, M. (2012) · Earth and Planetary Science Letters · doi:10.1016/j.epsl.2012.06.046 · Cited by 37
The composition of transiting giant extrasolar planets
Guillot, T. (2007) · HAL · Cited by 47
Extrasolar Planets: Constraints for Planet Formation Models
Santos, N. C., Benz, W., & Mayor, M. (2005) · Science · doi:10.1126/science.1100210 · Cited by 39
Self-citationMordasini, C., Klahr, H. H., Alibert, Y., Miller, N., & Henning, T. K. (2014) · doi:10.48550/arxiv.1403.5272 · Cited by 39
Self-citationPossible solution to the riddle of HD 82943 multiplanet system: the three-planet resonance 1:2:5?
Baluev, R., & Beaug'e, C. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt2486 · Cited by 13
AHerschelPACS survey of the dust and gas in Upper Scorpius disks
Mathews, G. S., Pinte, C., Duchêne, G., Williams, J. P., & Ménard, F. (2013) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201321228 · Cited by 38
Metallicity effect and planet mass function in pebble-based planet formation models
Brügger, N., Alibert, Y., Ataiee, S., & Benz, W. (2018) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201833347 · Cited by 38
Self-citationValletta, C., & Helled, R. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/aaf427 · Cited by 38
Flux-limited Diffusion Approximation Models of Giant Planet Formation by Disk Instability
Boss, A. (2008) · The Astrophysical Journal · doi:10.1086/533496 · Cited by 31
Formation and evolution of the two 4/3 resonant giants planets in HD 200964
dos Santos, M. T., Correa-Otto, J. A., Michtchenko, T. A., & Ferraz‐Mello, S. (2014) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201424820 · Cited by 37
Uribe, A., Klahr, H. H., & Henning, T. K. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/769/2/97 · Cited by 35
Maximum mass of planetary embryos that formed in core-accretion models
Alibert, Y. (2017) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/201630051/pdf · Cited by 37
Self-citationMousis, O. J., Guilbert-Lepoutre, A., Lunine, J. I., Cochran, A. L., Waite, J. H., Petit, J.-M., & Rousselot, P. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/757/2/146 · Cited by 37
Nayakshin, S., & Fletcher, M. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv1354 · Cited by 35
Setting the Stage: Planet Formation and Volatile Delivery
Venturini, J., Ronco, M. P., & Guilera, O. M. (2020) · Space Science Reviews · doi:10.1007/s11214-020-00700-y · Cited by 44
High resolution spectroscopy of stars with transiting planetsPreprint
Santos, N. C., Pont, F. J., Melo, C., Israelian, G., Bouchy, F., Mayor, M., Moutou, C., Queloz, D. P., Udry, S., & Guillot, T. (2006) · arXiv (Cornell University) · doi:10.1051/0004-6361:20054583 · Cited by 36
Alibert, Y., Mousis, O. J., & Benz, W. (2005) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20052841 · Cited by 55
Self-citationPrecise masses for the transiting planetary system HD 106315 with HARPS
Barros, S. C. C., Gosselin, H., Lillo-Box, J., Bayliss, D., Mena, E. D., Brugger, B., Santerne, A., Armstrong, D. J., Adibekyan, V., Armstrong, J. D., et al. (2017) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201731276 · Cited by 36
Atmosphere loss in planet–planet collisions
Denman, T. R., Leinhardt, Z. M., Carter, P. J., & Mordasini, C. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa1623 · Cited by 36
Self-citationPozuelos, F. J., Suárez, J. C., de Elía, G. C., Berdiñas, Z. M., Bonfanti, A., Dugaro, A., Gillon, M., Jehin, E., Günther, M. N., Grootel, V. V., et al. (2020) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/202038047/pdf · Cited by 36
The formation of Jupiter by hybrid pebble–planetesimal accretion
Alibert, Y., Venturini, J., Helled, R., Ataiee, S., Burn, R., Senecal, L. M. L., Benz, W., Mayer, L., Mordasini, C., Quanz, S. P., et al. (2018) · doi:10.7892/boris.128724 · Cited by 36
Self-citationHEAVY-ELEMENT ENRICHMENT OF A JUPITER-MASS PROTOPLANET AS A FUNCTION OF ORBITAL LOCATION
Helled, R., & Schubert, G. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/697/2/1256 · Cited by 20
Oligarchic planetesimal accretion and giant planet formation II
Fortier, A., Brunini, A., & Benvenuto, O. G. (2009) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/200811367/pdf · Cited by 36
Planetary population synthesis and the emergence of four classes of planetary system architectures
Emsenhuber, A., Mordasini, C., & Burn, R. (2023) · The European Physical Journal Plus · doi:10.1140/epjp/s13360-023-03784-x · Cited by 41
Self-citationAN ALMA CONSTRAINT ON THE GSC 6214-210 B CIRCUM-SUBSTELLAR ACCRETION DISK MASS
Bowler, B., Andrews, S., Kraus, A., Ireland, M., Herczeg, G., Ricci, L., Carpenter, J., & Brown, M. E. (2015) · The Astrophysical Journal Letters · doi:10.1088/2041-8205/805/2/l17 · Cited by 28
The Exoplanet Population Observation Simulator. II -- Population Synthesis in the Era of Kepler
Mulders, G. D., Mordasini, C., Pascucci, I., Ciesla, F. J., Emsenhuber, A., & Apai, D. (2019) · Bern Open Repository and Information System (University of Bern) · doi:10.48550/arxiv.1905.08804 · Cited by 35
Self-citationJupiter’s formation and its primordial internal structure
Lozovsky, M., Helled, R., Rosenberg, E. D., & Bodenheimer, P. H. (2017) · Zurich Open Repository and Archive (University of Zurich) · doi:10.5167/uzh-143117 · Cited by 35
Lithium abundances in exoplanet-host stars: modelling
Castro, M., Vauclair, S. D., Richard, O., & Santos, N. C. (2008) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20078928 · Cited by 35
The growth and migration of massive planets under the influence of external photoevaporation
Winter, A. J., Haworth, T. J., Coleman, G. A. L., & Nayakshin, S. (2022) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stac1564 · Cited by 34
Outward transport of CAIs during FU‐Orionis events
Wurm, G., & Haack, H. (2009) · Meteoritics and Planetary Science · doi:10.1111/j.1945-5100.2009.tb00763.x · Cited by 34
SEARCH FOR GAMMA RAY BURSTS WITH THE ARGO-YBJ DETECTOR IN SCALER MODE
Aielli, G., Bacci, C., Barone, F., Bartoli, B., Bernardini, P., Bi, X.-J., Bleve, C., Branchini, P., Budano, A., Bussino, S., et al. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/699/2/1281 · Cited by 33
THE ROLE OF METHANOL IN THE CRYSTALLIZATION OF TITAN'S PRIMORDIAL OCEAN
Deschamps, F., Mousis, O. J., Sanchez‐Valle, C., & Lunine, J. I. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/724/2/887 · Cited by 34
Growth of Jupiter: Enhancement of core accretion by a voluminous low-mass envelope
D’Angelo, G., WEIDENSCHILLING, S. J., Lissauer, J. J., & Bodenheimer, P. H. (2014) · Icarus · doi:10.1016/j.icarus.2014.06.029 · Cited by 33
Chemical fingerprints of hot Jupiter planet formation
Maldonado, J., Villaver, E., & Eiroa, C. (2017) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201732001 · Cited by 34
From planetesimals to planets: volatile molecules
Marboeuf, U., Thiabaud, A., Alibert, Y., Cabral, N., & Benz, W. (2014) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/201423431/pdf · Cited by 33
Self-citationGlobal 3D radiation hydrodynamic simulations of proto-Jupiter’s convective envelope
Zhu, Z., Jiang, Y.-F., Baehr, H. D., Youdin, A. N., Armitage, P. J., & Martin, R. G. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab2517 · Cited by 33
Dust settling and rapid planetary migration
Hasegawa, Y., & Pudritz, R. E. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.18135.x · Cited by 32
Giant planet population synthesis: comparing theory with observations
Benz, W., Mordasini, C., Alibert, Y., & Naef, D. (2008) · Physica Scripta · doi:10.1088/0031-8949/2008/t130/014022 · Cited by 32
Self-citationA SCUBA-2 850-μm survey of protoplanetary discs in the σ Orionis cluster
Williams, J. P., Cieza, L. A., Andrews, S. M., Coulson, I. M., Barger, A. J., Casey, C. M., Chen, C.-C., Cowie, L. L., Koss, M., Lee, N., et al. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt1407 · Cited by 31
A Comparative Study of WASP-67 b and HAT-P-38 b from WFC3 Data
Bruno, G., Lewis, N. K., Stevenson, K. B., Filippazzo, J., Hill, M., Fraine, J., Wakeford, H. R., Deming, D., Kilpatrick, B., Line, M. R., et al. (2018) · The Astronomical Journal · doi:10.3847/1538-3881/aaa0c7 · Cited by 29
Circumstellar disks and planets
Wolf, S., Malbet, F., Alexander, R. D., Berger, J.-P., Creech-Eakman, M. J., Duchêne, G., Dutrey, A., Mordasini, C., Pantin, E., Pont, F. J., et al. (2012) · The Astronomy and Astrophysics Review · doi:10.1007/s00159-012-0052-1 · Cited by 32
Self-citationMost super-Earths formed by dry pebble accretion are less massive than 5 Earth masses
Venturini, J., Guilera, O. M., Ronco, M. P., & Mordasini, C. (2020) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/202039140/pdf · Cited by 32
Self-citationBowens, R., Meyer, M. R., Delacroix, C., Absil, O., van Boekel, R., Quanz, S. P., Shinde, M., Kenworthy, M. A., Carlomagno, B., de Xivry, G. O., et al. (2021) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202141109 · Cited by 35
Nonlinear Dynamical Friction in a Gaseous MediumPreprint
Kim, H., & Kim, W. (2012) · Cited by 32
Formation of hot Jupiters through disk migration and evolving stellar tides
Heller, R. (2019) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201833486 · Cited by 38
The Origin of the Heavy-element Content Trend in Giant Planets via Core Accretion
Hasegawa, Y., Bryden, G., Ikoma, M., Vasisht, G., & Swain, M. G. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aad912 · Cited by 32
Oligarchic planetesimal accretion and giant planet formation II
Fortier, A., Benvenuto, O. G., & Brunini, A. (2009) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200811367 · Cited by 31
Critical core masses for gas giant formation with grain-free envelopesPreprint
Hori, Y., & Ikoma, M. (2010) · Cited by 31
Valletta, C., & Helled, R. (2019) · Zurich Open Repository and Archive (University of Zurich) · doi:10.5167/uzh-182778 · Cited by 30
Setting the stage: Planet formation and volatile delivery
Venturini, J., Ronco, M. P., & Guilera, O. M. (2020) · Conicet · Cited by 30
Liu, B., Zhang, X., Lin, D. N. C., & Aarseth, S. J. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/798/1/62 · Cited by 30
Water and Volatiles in the Outer Solar System
Grasset, O., Castillo-Rogez, J. C., Guillot, T., Fletcher, L. N., & Tosi, F. (2017) · Space Science Reviews · doi:10.1007/s11214-017-0407-z · Cited by 33
Rayleigh adjustment of narrow barriers in protoplanetary discs
Yang, C.-C., & Kristen Menou, A. (2009) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.16047.x · Cited by 30
Rice, K., Penny, M. T., & Horne, K. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sts079 · Cited by 29
Searching for Giant Exoplanets around M-dwarf Stars (GEMS) I: Survey Motivation
Kanodia, S., Cañas, C., Mahadevan, S., Ford, E. B., Helled, R., Anderson, D. E., Boss, A., Cochran, W., Delamer, M., Han, T., et al. (2024) · Astronomical Journal · doi:10.3847/1538-3881/ad27cb · Cited by 28
Merger by migration at the final phase of common envelope evolution
Soker, N. (2012) · New Astronomy · doi:10.1016/j.newast.2012.05.001 · Cited by 29
Magnetic topologies of young suns: the weak-line T Tauri stars TWA 6 and TWA 8A
Hill, C. A., Folsom, C. P., Donati, J. ‐., Herczeg, G. J., Hussain, G. A. J., Alencar, S. H. P., & Gregory, S. G. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz403 · Cited by 31
Takaishi, D., Tsukamoto, Y., & Suto, Y. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa179 · Cited by 28
Microlensing Results Challenge the Core Accretion Runaway Growth Scenario for Gas Giants
Suzuki, D., Bennett, D. P., Ida, S., Mordasini, C., Bhattacharya, A., Bond, I. A., Donachie, M., Fukui, A., Hirao, Y., Koshimoto, N., et al. (2018) · doi:10.7892/boris.128661 · Cited by 29
Self-citationGENGA. II. GPU Planetary N-body Simulations with Non-Newtonian Forces and High Number of Particles
Grimm, S. L., Stadel, J., Brasser, R., MEIER, M. M. M., & Mordasini, C. (2022) · The Astrophysical Journal · doi:10.3847/1538-4357/ac6dd2 · Cited by 29
Self-citationSubstellar Companions to Evolved Intermediate-Mass Stars: HD 145457 and HD 180314
Sato, B., Omiya, M., Yujuan, L., Harakawa, H., Izumiura, H., Kambe, E., Toyota, E., Murata, D., Lee, B., Masuda, S., et al. (2010) · Institutional Repositories DataBase (IRDB) · Cited by 29
Theoretical models of planetary system formation
Pfyffer, S., Alibert, Y., Benz, W., & Swoboda, D. (2015) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201424295 · Cited by 29
Self-citationIs There a Temperature Limit in Planet Formation at 1000 K?
Demirci, T., Teiser, J., Steinpilz, T., Landers, J., Salamon, S., Wende, H., & Wurm, G. (2017) · The Astrophysical Journal · doi:10.3847/1538-4357/aa816c · Cited by 28
Galvagni, M., & Mayer, L. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt2108 · Cited by 28
APPLE: An Evolution Code for Modeling Giant Planets
Sur, A., Su, Y., Arevalo, R. A. T., Chen, Y.-X., & Burrows, A. S. (2024) · The Astrophysical Journal · doi:10.3847/1538-4357/ad57c3 · Cited by 27
Díaz, R. F., Santerne, A., Sahlmann, J., Hébrard, G., Eggenberger, A., Santos, N. C., Moutou, C., Arnold, L., Boisse, I., Bonfils, X., et al. (2011) · Archive ouverte UNIGE (University of Geneva) · doi:10.48550/arxiv.1111.1168 · Cited by 27
K2-114b and K2-115b: Two Transiting Warm Jupiters
Shporer, A., Zhou, G., Fulton, B. J., Vanderburg, A. M., Espinoza, N., Collins, K. A., Ciardi, D. R., Bayliss, D., Armstrong, J. D., Bento, J. D. S., et al. (2017) · The Astronomical Journal · doi:10.3847/1538-3881/aa8bb9 · Cited by 21
Formation of planetary populations – I. Metallicity and envelope opacity effects
Alessi, M., & Pudritz, R. E. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty1170 · Cited by 27
Toward a population synthesis of disks and planets
Emsenhuber, A., Burn, R., Weder, J., Monsch, K., Picogna, G., Ercolano, B., & Preibisch, T. (2023) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202244767 · Cited by 27
The growth and hydrodynamic collapse of a protoplanet envelopePreprint
Ayliffe, B. A., & Bate, M. R. (2012) · Cited by 27
Combing the brown dwarf desert with Gaia DR3
Stevenson, A. T., Haswell, C. A., Barnes, J. R., & Barstow, J. K. (2023) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stad3041 · Cited by 26
Egger, J. A., Osborn, H. P., Kubyshkina, D. I., Mordasini, C., Alibert, Y., Günther, M. N., Lendl, M., Brandeker, A., Heitzmann, A., Leleu, A., et al. (2024) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202450472 · Cited by 26
Self-citationA METHOD TO CONSTRAIN THE SIZE OF THE PROTOSOLAR NEBULA
Kretke, K. A., Levison, H. F., Buie, M. W., & Morbidelli, A. (2012) · The Astronomical Journal · doi:10.1088/0004-6256/143/4/91 · Cited by 25
In situ formation of hot Jupiters with companion super-Earths
Poon, S. T. S., Nelson, R. P., & Coleman, G. A. L. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab1466 · Cited by 27
Small Protoplanetary Disks in the Orion Nebula Cluster and OMC1 with ALMA
Otter, J. A., Ginsburg, A. G., Ballering, N. P., Bally, J., Eisner, J. A., Goddi, C., Plambeck, R. L., & Wright, M. C. H. (2021) · The Astrophysical Journal · doi:10.3847/1538-4357/ac29c2 · Cited by 26
Trapping planets in an evolving protoplanetary disk: preferred time, locations, and planet mass
Baillié, K., Charnoz, S., & Pantin, E. (2016) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201528027 · Cited by 26
Using deep neural networks to compute the mass of forming planets
Alibert, Y., & Venturini, J. (2019) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201834942 · Cited by 26
Self-citationFormation via Disk Instability
Mayer, L. (2010) · Wiley eBooks · doi:10.1002/9783527629763.ch4 · Cited by 26
Envelope instability in giant planet formation
Benvenuto, O. G., Brunini, A., & Fortier, A. (2007) · Icarus · doi:10.1016/j.icarus.2007.06.019 · Cited by 25
Rapid formation of gas giants, ice giants and super-Earths
Boss, A. (2008) · Physica Scripta · doi:10.1088/0031-8949/2008/t130/014020 · Cited by 7
Chemical analysis of early-type stars with planets
Saffe, C., Miquelarena, P., Alacoria, J., Flores, M., Arancibia, M. J., Calvo, D., Girardi, G., Grosso, M., & Collado, A. E. (2021) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202040132 · Cited by 25
Ronco, M. P., Guilera, O. M., Cuadra, J., Bertolami, M. M. M., Cuello, N., Fontecilla, C., Poblete, P. P., & Bayo, A. (2021) · The Astrophysical Journal · doi:10.3847/1538-4357/ac0438 · Cited by 25
Framework for the architecture of exoplanetary systems
Mishra, L., Alibert, Y., Udry, S., & Mordasini, C. (2023) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202244705 · Cited by 32
Self-citationEffects of photophoresis on the evolution of transitional circumstellar disks
Herrmann, F., & Krivov, A. V. (2007) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20078322 · Cited by 25
Metadata
- Authors
- Alibert, Y., Mordasini, C., Benz, W., & Winisdoerffer, C.
- Affiliations
- University of Bern (CH)
- University of Leicester (GB)
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2005-04
- Volume
- 434
- Issue
- 1
- Pages
- 343-353
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W2134475956
- Cited by
- 685
- References
- 52
- Citations by year
- 2026: 20 · 2025: 19 · 2024: 23 · 2023: 20 · 2022: 27 · 2021: 32 · 2020: 37 · 2019: 38 · 2018: 36 · 2017: 34 · 2016: 34 · 2015: 30 · 2014: 37 · 2013: 26 · 2012: 39
- FWCI
- 23.64
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- Astronomy and Astrophysics (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- Springer Link (Chiba Institute of Technology) (submittedVersion)
- Bern Open Repository and Information System (University of Bern) (submittedVersion)
- CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
- arXiv (Cornell University)
- Funders
- National Science Foundation
- Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung
- Topics
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Keywords
- giant planet formation, core accretion, planet migration, protoplanetary disc evolution, gap formation, disc lifetime, semi-major axis, exoplanets, planetary mass
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
