Why do protoplanetary disks appear not massive enough to form the known exoplanet population?
A&A, 618 (2018) L3
Published online: 2018-10-11
Articles citing this article
The Citing articles tool gives a list of articles citing the current article.
The citing articles come from EDP Sciences database, as well as other publishers participating in CrossRef Cited-by Linking Program. You can set up your personal account to receive an email alert each time this article is cited by a new article (see the menu on the right-hand side of the abstract page).
Cited article:
This article has been cited by the following article(s):
Modeling the Protoplanetary Disks of Two Brown Dwarfs in the Taurus Molecular Cloud
Anneliese M. Rilinger, Catherine C. Espaillat and Enrique MacíasThe Astrophysical Journal 878 (2) 103 (2019)
https://doi.org/10.3847/1538-4357/ab211d
New Constraints From Dust Lines on the Surface Densities of Protoplanetary Disks
Diana Powell, Ruth Murray-Clay, Laura M. Pérez, Hilke E. Schlichting and Mickey RosenthalThe Astrophysical Journal 878 (2) 116 (2019)
https://doi.org/10.3847/1538-4357/ab20ce
The Temporal Requirements of Directly Observing Self-gravitating Spiral Waves in Protoplanetary Disks with ALMA
Cassandra Hall, Ruobing Dong, Ken Rice, Tim J. Harries, Joan Najita, Richard Alexander and Sean BrittainThe Astrophysical Journal 871 (2) 228 (2019)
https://doi.org/10.3847/1538-4357/aafac2
Constraining disk evolution prescriptions of planet population synthesis models with observed disk masses and accretion rates
C. F. Manara, C. Mordasini, L. Testi, et al.Astronomy & Astrophysics 631 L2 (2019)
https://doi.org/10.1051/0004-6361/201936488
Exploring the conditions for forming cold gas giants through planetesimal accretion
Anders Johansen and Bertram BitschAstronomy & Astrophysics 631 A70 (2019)
https://doi.org/10.1051/0004-6361/201936351
Formation of planetary systems by pebble accretion and migration
Michiel Lambrechts, Alessandro Morbidelli, Seth A. Jacobson, et al.Astronomy & Astrophysics 627 A83 (2019)
https://doi.org/10.1051/0004-6361/201834229
The Ophiuchus DIsk Survey Employing ALMA (ODISEA): Disk Dust Mass Distributions across Protostellar Evolutionary Classes
Jonathan P. Williams, Lucas Cieza, Antonio Hales, Megan Ansdell, Dary Ruiz-Rodriguez, Simon Casassus, Sebastian Perez and Alice ZurloThe Astrophysical Journal Letters 875 (2) L9 (2019)
https://doi.org/10.3847/2041-8213/ab1338
Bright C2H emission in protoplanetary discs in Lupus: high volatile C/O > 1 ratios
A. Miotello, S. Facchini, E. F. van Dishoeck, et al.Astronomy & Astrophysics 631 A69 (2019)
https://doi.org/10.1051/0004-6361/201935441
A multi-scale exploration of a massive young stellar object
A. J. Frost, R. D. Oudmaijer, W. J. de Wit and S. L. LumsdenAstronomy & Astrophysics 625 A44 (2019)
https://doi.org/10.1051/0004-6361/201834583
Classical T-Tauri stars with VPHAS+: II: NGC 6383 in Sh 2-012★
V M KalariMonthly Notices of the Royal Astronomical Society 484 (4) 5102 (2019)
https://doi.org/10.1093/mnras/stz250
The Gemini Planet Imager Exoplanet Survey: Giant Planet and Brown Dwarf Demographics from 10 to 100 au
Eric L. Nielsen, Robert J. De Rosa, Bruce Macintosh, Jason J. Wang, Jean-Baptiste Ruffio, Eugene Chiang, Mark S. Marley, Didier Saumon, Dmitry Savransky, S. Mark Ammons, Vanessa P. Bailey, Travis Barman, Célia Blain, Joanna Bulger, Adam Burrows, Jeffrey Chilcote, Tara Cotten, Ian Czekala, Rene Doyon, Gaspard Duchêne, Thomas M. Esposito, Daniel Fabrycky, Michael P. Fitzgerald, Katherine B. Follette, Jonathan J. Fortney, et al.The Astronomical Journal 158 (1) 13 (2019)
https://doi.org/10.3847/1538-3881/ab16e9
Formation of planetary systems by pebble accretion and migration: growth of gas giants
Bertram Bitsch, Andre Izidoro, Anders Johansen, et al.Astronomy & Astrophysics 623 A88 (2019)
https://doi.org/10.1051/0004-6361/201834489
External photoevaporation of circumstellar discs constrains the time-scale for planet formation
Francisca Concha-Ramírez, Martijn J C Wilhelm, Simon Portegies Zwart and Thomas J HaworthMonthly Notices of the Royal Astronomical Society 490 (4) 5678 (2019)
https://doi.org/10.1093/mnras/stz2973
Newborn stars don’t have enough dust to build planets. What are the missing ingredients?
Nola Taylor ReddProceedings of the National Academy of Sciences 116 (16) 7605 (2019)
https://doi.org/10.1073/pnas.1904572116
On the millimetre continuum flux–radius correlation of proto-planetary discs
Giovanni P Rosotti, Richard A Booth, Marco Tazzari, Cathie Clarke, Giuseppe Lodato and Leonardo TestiMonthly Notices of the Royal Astronomical Society: Letters 486 (1) L63 (2019)
https://doi.org/10.1093/mnrasl/slz064
These dusty young stars are changing the rules of planet-building
Rebecca BoyleNature 564 (7734) 20 (2018)
https://doi.org/10.1038/d41586-018-07591-8