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).
This article has been cited by the following article(s):
Protoplanetary Disk Size under Nonideal Magnetohydrodynamics: A General Formalism with Inclined Magnetic Field
Yueh-Ning 悅寧 Lee 李, Barshan Ray, Pierre Marchand and Patrick Hennebelle The Astrophysical Journal Letters 961(2) L28 (2024) https://doi.org/10.3847/2041-8213/ad192a
The Physical Origin of the Stellar Initial Mass Function
Wide-binary eccentricity distribution in young star clusters: dependence on the binary separation and mass
Sajay Sunny Mathew, Siyao Xu, Christoph Federrath, Yue Hu and Amit Seta Monthly Notices of the Royal Astronomical Society 532(2) 2374 (2024) https://doi.org/10.1093/mnras/stae1632
Synthetic populations of protoplanetary disks: Impact of magnetic fields and radiative transfer
U. Lebreuilly, P. Hennebelle, T. Colman, A. Maury, N. D. Tung, L. Testi, R. Klessen, S. Molinari, B. Commerçon, M. González, E. Pacetti, A. Somigliana and G. Rosotti Astronomy & Astrophysics 682 A30 (2024) https://doi.org/10.1051/0004-6361/202346558
Massive pre-stellar cores in radiation-magneto-turbulent simulations of molecular clouds
Simulating ionization feedback from young massive stars: impact of numerical resolution
Yunwei Deng, Hui Li, Rahul Kannan, Aaron Smith, Mark Vogelsberger and Greg L Bryan Monthly Notices of the Royal Astronomical Society 527(1) 478 (2023) https://doi.org/10.1093/mnras/stad3202
Influence of magnetic field and stellar radiative feedback on the collapse and the stellar mass spectrum of a massive star-forming clump
Star cluster formation in clouds with externally driven turbulence
Jamie D Smith, James E Dale, Sarah E Jaffa and Martin G H Krause Monthly Notices of the Royal Astronomical Society 516(3) 4212 (2022) https://doi.org/10.1093/mnras/stac2295
Less wrong: a more realistic initial condition for simulations of turbulent molecular clouds
Henry B Lane, Michael Y Grudić, Dávid Guszejnov, et al. Monthly Notices of the Royal Astronomical Society 510(4) 4767 (2022) https://doi.org/10.1093/mnras/stab3739
The role of the turbulence driving mode for the initial mass function
Sajay Sunny Mathew, Christoph Federrath and Amit Seta Monthly Notices of the Royal Astronomical Society 518(4) 5190 (2022) https://doi.org/10.1093/mnras/stac3415
On the origin of magnetic fields in stars – II. The effect of numerical resolution
James Wurster, Matthew R Bate, Daniel J Price and Ian A Bonnell Monthly Notices of the Royal Astronomical Society 511(1) 746 (2022) https://doi.org/10.1093/mnras/stac123
STARFORGE: Towards a comprehensive numerical model of star cluster formation and feedback
Michael Y Grudić, Dávid Guszejnov, Philip F Hopkins, Stella S R Offner and Claude-André Faucher-Giguère Monthly Notices of the Royal Astronomical Society 506(2) 2199 (2021) https://doi.org/10.1093/mnras/stab1347
Amplification and generation of turbulence during self-gravitating collapse
Do fragmentation and accretion affect the stellar initial mass function?
R S Klessen, S Vanaverbeke, D R G Schleicher and R Riaz Monthly Notices of the Royal Astronomical Society 494(2) 1647 (2020) https://doi.org/10.1093/mnras/staa787
When H ii regions are complicated: considering perturbations from winds, radiation pressure, and other effects
Sam Geen, Eric Pellegrini, Rebekka Bieri and Ralf Klessen Monthly Notices of the Royal Astronomical Society 492(1) 915 (2020) https://doi.org/10.1093/mnras/stz3491
Can magnetized turbulence set the mass scale of stars?
Dávid Guszejnov, Michael Y Grudić, Philip F Hopkins, Stella S R Offner and Claude-André Faucher-Giguère Monthly Notices of the Royal Astronomical Society 496(4) 5072 (2020) https://doi.org/10.1093/mnras/staa1883
Erratum: Can magnetized turbulence set the mass scale of stars?
Dávid Guszejnov, Michael Y Grudić, Philip F Hopkins, Stella S R Offner and Claude-André Faucher-Giguère Monthly Notices of the Royal Astronomical Society 500(1) 1125 (2020) https://doi.org/10.1093/mnras/staa3413
On the origin of the peak of the stellar initial mass function: exploring the tidal screening theory
There is no magnetic braking catastrophe: low-mass star cluster and protostellar disc formation with non-ideal magnetohydrodynamics
James Wurster, Matthew R Bate and Daniel J Price Monthly Notices of the Royal Astronomical Society 489(2) 1719 (2019) https://doi.org/10.1093/mnras/stz2215
The Role of Magnetic Field in Molecular Cloud Formation and Evolution
Simulating star clusters across cosmic time – I. Initial mass function, star formation rates, and efficiencies
Chong-Chong He, Massimo Ricotti and Sam Geen Monthly Notices of the Royal Astronomical Society 489(2) 1880 (2019) https://doi.org/10.1093/mnras/stz2239
How First Hydrostatic Cores, Tidal Forces, and Gravoturbulent Fluctuations Set the Characteristic Mass of Stars
The Unusual Initial Mass Function of the Arches Cluster
Matthew W. Hosek, Jessica R. Lu, Jay Anderson, Francisco Najarro, Andrea M. Ghez, Mark R. Morris, William I. Clarkson and Saundra M. Albers The Astrophysical Journal 870(1) 44 (2019) https://doi.org/10.3847/1538-4357/aaef90
Stellar mass spectrum within massive collapsing clumps
A dual power-law distribution for the stellar initial mass function
Karl Heinz Hoffmann, Christopher Essex, Shantanu Basu and Janett Prehl Monthly Notices of the Royal Astronomical Society 478(2) 2113 (2018) https://doi.org/10.1093/mnras/sty1251