Citation Impact

Citing Papers

Nature of the Galactic centre NIR-excess sources
2017
Feedback by massive stars and the emergence of superbubbles
2012
Dust-enshrouded star near supermassive black hole: predictions for high-eccentricity passages near low-luminosity galactic nuclei
2014
The kinematics and dark matter fractions of TNG50 galaxies at z = 2 from an observational perspective
2020 StandoutNobel
How to model supernovae in simulations of star and galaxy formation
2018
DETECTION OF GALACTIC CENTER SOURCE G2 AT 3.8 μm DURING PERIAPSE PASSAGE
2014 StandoutNobel
Feedback by massive stars and the emergence of superbubbles - I. Energy efficiency and Vishniac instabilities
2013
THE PLUTO CODE FOR ADAPTIVE MESH COMPUTATIONS IN ASTROPHYSICAL FLUID DYNAMICS
2011
Magnetic Reconnection and Hot Spot Formation in Black Hole Accretion Disks
2020
Sgr A* near-infrared flares from reconnection events in a magnetically arrested disc
2020 StandoutNobel
3D AMR hydrosimulations of a compact-source scenario for the Galactic Centre cloud G2
2018 StandoutNobel
3D ADAPTIVE MESH REFINEMENT SIMULATIONS OF THE GAS CLOUD G2 BORN WITHIN THE DISKS OF YOUNG STARS IN THE GALACTIC CENTER
2015 StandoutNobel
Detection of a Drag Force in G2's Orbit: Measuring the Density of the Accretion Flow onto Sgr A* at 1000 Schwarzschild Radii
2019 StandoutNobel
The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations
2015 Standout
Effect of an isotropic outflow from the Galactic Centre on the bow-shock evolution along the orbit
2015

Works of Z. Méliani being referenced

COMPUTING THE DUST DISTRIBUTION IN THE BOW SHOCK OF A FAST-MOVING, EVOLVED STAR
2011
A multidimensional grid-adaptive relativistic magnetofluid code
2008
A hydrodynamical model of the circumstellar bubble created by two massive stars
2012
A far-infrared survey of bow shocks and detached shells around AGB stars and red supergiants
2011
Can the magnetic field in the Orion arm inhibit the growth of instabilities in the bow shock of Betelgeuse?
2014
Rankless by CCL
2026