61 citations · 305 across the 10 of their papers we have counts for
24 papers
The AGORA High-resolution Galaxy Simulations Comparison Project. III: Cosmological zoom-in simulation of a Milky Way-mass halo
Santi Roca-Fàbrega, Ji-hoon Kim, Loic Hausammann +20
We present a suite of high-resolution cosmological zoom-in simulations to of a halo at , obtained using seven contemporary astrophysical simul…
Chemical analysis of prestellar cores in Ophiuchus yields short timescales and rapid collapse
Stefano Bovino, Alessandro Lupi, Andrea Giannetti +4
Sun-like stars form from the contraction of cold and dense interstellar clouds. How the collapse proceeds and what are the main physical processes driving it, however, is still und…
Chemical post-processing of magneto-hydrodynamical simulations of star-forming regions: robustness and pitfalls
Simón Ferrada-Chamorro, Alessandro Lupi, Stefano Bovino
A common approach to model complex chemistry in numerical simulations is via post-processing of existing magneto-hydrodynamic simulations, relying on computing the evolution of che…
Constraints on the [CII] luminosity of a proto-globular cluster at z~6 obtained with ALMA
F. Calura, E. Vanzella, S. Carniani +11
We report on ALMA observations of D1, a system at z~6.15 with stellar mass M_* ~ 10^7 M_sun containing globular cluster (GC) precursors, strongly magnified by the galaxy cluster MA…
Dynamical evolution of massive perturbers in realistic multi-component galaxy models I: implementation and validation
Matteo Bonetti, Elisa Bortolas, Alessandro Lupi +1
Galaxies are self-gravitating structures composed by several components encompassing spherical, axial and triaxial symmetry. Although real systems feature heterogeneous components…
Missing [CII] emission from early galaxies
S. Carniani, A. Ferrara, R. Maiolino +9
ALMA observations have revealed that [CII] 158m line emission in high-z galaxies is ~2-3 more extended than the UV continuum emission. Here we explore whether surface br…