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):
TRACKING THE DISTRIBUTION OF 26Al AND 60Fe DURING THE EARLY PHASES OF STAR AND DISK EVOLUTION
Michael Kuffmeier, Troels Frostholm Mogensen, Troels Haugbølle, Martin Bizzarro and Åke Nordlund The Astrophysical Journal 826(1) 22 (2016) https://doi.org/10.3847/0004-637X/826/1/22
MAGNETICALLY SELF-REGULATED FORMATION OF EARLY PROTOPLANETARY DISKS
Cosmic Dawn (CoDa): the first radiation-hydrodynamics simulation of reionization and galaxy formation in the Local Universe
Pierre Ocvirk, Nicolas Gillet, Paul R. Shapiro, et al. Monthly Notices of the Royal Astronomical Society 463(2) 1462 (2016) https://doi.org/10.1093/mnras/stw2036
CLUSTERS OF SMALL CLUMPS CAN EXPLAIN THE PECULIAR PROPERTIES OF GIANT CLUMPS IN HIGH-REDSHIFT GALAXIES
New insights on the spin-up of a neutron star during core collapse
Rémi Kazeroni, Jérôme Guilet and Thierry Foglizzo Monthly Notices of the Royal Astronomical Society 456(1) 126 (2016) https://doi.org/10.1093/mnras/stv2666
An implicit scheme for solving the anisotropic diffusion of heat and cosmic rays in the RAMSES code
The stress–pressure relationship in simulations of MRI-induced turbulence
Johnathan Ross, Henrik N. Latter and Jerome Guilet Monthly Notices of the Royal Astronomical Society 455(1) 526 (2016) https://doi.org/10.1093/mnras/stv2286
Local and global aspects of the linear MRI in accretion discs
Henrik N. Latter, Sebastien Fromang and Julien Faure Monthly Notices of the Royal Astronomical Society 453(3) 3258 (2015) https://doi.org/10.1093/mnras/stv1890
Galaxy evolution: modelling the role of non-thermal pressure in the interstellar medium
Yuval Birnboim, Shmuel Balberg and Romain Teyssier Monthly Notices of the Royal Astronomical Society 447(4) 3678 (2015) https://doi.org/10.1093/mnras/stu2717
Grid-based Methods in Relativistic Hydrodynamics and Magnetohydrodynamics
Photoionization feedback in a self-gravitating, magnetized, turbulent cloud
Sam Geen, Patrick Hennebelle, Pascal Tremblin and Joakim Rosdahl Monthly Notices of the Royal Astronomical Society 454(4) 4484 (2015) https://doi.org/10.1093/mnras/stv2272
Vortex cycles at the inner edges of dead zones in protoplanetary disks
T. G. Bisbas, T. J. Haworth, R. J. R. Williams, et al. Monthly Notices of the Royal Astronomical Society 453(2) 1324 (2015) https://doi.org/10.1093/mnras/stv1659
Polarized thermal dust emission as seen by Planck : A comparison with MHD simulations and lessons from a toy model
Baryonic and dark matter distribution in cosmological simulations of spiral galaxies
Pol Mollitor, Emmanuel Nezri and Romain Teyssier Monthly Notices of the Royal Astronomical Society 447(2) 1353 (2015) https://doi.org/10.1093/mnras/stu2466
Brightest cluster galaxies in cosmological simulations with adaptive mesh refinement: successes and failures
Davide Martizzi, Jimmy, Romain Teyssier and Ben Moore Monthly Notices of the Royal Astronomical Society 443(2) 1500 (2014) https://doi.org/10.1093/mnras/stu1233
Simulations of magnetized multiphase galactic disc regulated by supernovae explosions
A systematic look at the effects of radiative feedback on disc galaxy formation
Rok Roškar, Romain Teyssier, Oscar Agertz, Markus Wetzstein and Ben Moore Monthly Notices of the Royal Astronomical Society 444(3) 2837 (2014) https://doi.org/10.1093/mnras/stu1548
The biasing of baryons on the cluster mass function and cosmological parameter estimation
Davide Martizzi, Irshad Mohammed, Romain Teyssier and Ben Moore Monthly Notices of the Royal Astronomical Society 440(3) 2290 (2014) https://doi.org/10.1093/mnras/stu440
Cosmic rays as regulators of molecular cloud properties
Marc Joos, Patrick Hennebelle and Andrea Ciardi Astrophysics and Space Science Proceedings, The Labyrinth of Star Formation 36 69 (2014) https://doi.org/10.1007/978-3-319-03041-8_12
A discontinuous Galerkin method for solving the fluid and magnetohydrodynamic equations in astrophysical simulations
Philip Mocz, Mark Vogelsberger, Debora Sijacki, Rüdiger Pakmor and Lars Hernquist Monthly Notices of the Royal Astronomical Society 437(1) 397 (2014) https://doi.org/10.1093/mnras/stt1890
Cusp–core transformations induced by AGN feedback in the progenitors of cluster galaxies
Davide Martizzi, Romain Teyssier and Ben Moore Monthly Notices of the Royal Astronomical Society 432(3) 1947 (2013) https://doi.org/10.1093/mnras/stt297
DR 21(OH): A HIGHLY FRAGMENTED, MAGNETIZED, TURBULENT DENSE CORE
Cusp-core transformations in dwarf galaxies: observational predictions
Romain Teyssier, Andrew Pontzen, Yohan Dubois and Justin I. Read Monthly Notices of the Royal Astronomical Society 429(4) 3068 (2013) https://doi.org/10.1093/mnras/sts563
Transport of magnetic flux and the vertical structure of accretion discs – II. Vertical profile of the diffusion coefficients
Type I planet migration in weakly magnetized laminar discs
Jérôme Guilet, Clément Baruteau and John C. B. Papaloizou Monthly Notices of the Royal Astronomical Society 430(3) 1764 (2013) https://doi.org/10.1093/mnras/sts720
The influence of turbulence during magnetized core collapse and its consequences on low-mass star formation
INCORPORATING AMBIPOLAR AND OHMIC DIFFUSION IN THE AMR MHD CODE RAMSES
J. Masson, R. Teyssier, C. Mulet-Marquis, P. Hennebelle and G. Chabrier The Astrophysical Journal Supplement Series 201(2) 24 (2012) https://doi.org/10.1088/0067-0049/201/2/24
The effects of baryon physics, black holes and active galactic nucleus feedback on the mass distribution in clusters of galaxies
Type I Planet Migration in Weakly Magnetized Laminar Disks
Jérôme Guilet, Clément Baruteau and John C. B. Papaloizou Proceedings of the International Astronomical Union 8(S293) 256 (2012) https://doi.org/10.1017/S1743921313012945
Filaments and sheets of the warm-hot intergalactic medium
A STABLE, ACCURATE METHODOLOGY FOR HIGH MACH NUMBER, STRONG MAGNETIC FIELD MHD TURBULENCE WITH ADAPTIVE MESH REFINEMENT: RESOLUTION AND REFINEMENT STUDIES