254 citations · 4k across the 119 of their papers we have counts for
7 papers · 2 filters
The ALMA-ALPINE [CII] survey: sub-kpc morphology of 3 main-sequence galaxy systems at z~4.5 revealed by ALMA
T. Devereaux, P. Cassata, E. Ibar +25
Context: From redshift 6 to redshift 4 galaxies grow rapidly from low mass galaxies towards the more mature massive galaxies we see at the cosmic noon. Growth via gas acc…
The ALMA-ALPINE [CII] survey: Kennicutt-Schmidt relation in four massive main-sequence galaxies at z~4.5
M. Béthermin, C. Accard, C. Guillaume +40
The Kennicutt-Schmidt (KS) relation between the gas and the star formation rate (SFR) surface density (-) is essential to understand star formation proces…
Properties of the Magellanic Corona
Scott Lucchini, Elena D'Onghia, Andrew J. Fox
We characterize the Magellanic Corona, the warm gaseous halo around the Large Magellanic Cloud (LMC). The Corona is a key ingredient in the formation of the Magellanic Stream (Lucc…
Atomic Hydrogen Shows its True Colours: Correlations between HI and Galaxy Colour in Simulations
Calvin Osinga, Benedikt Diemer, Francisco Villaescusa-Navarro +2
Intensity mapping experiments are beginning to measure the spatial distribution of neutral atomic hydrogen (HI) to constrain cosmological parameters and the large-scale distributio…
The Milky Way Bar Pattern Speed using Hercules and Gaia DR3
Scott Lucchini, Elena D'Onghia, J. Alfonso L. Aguerri
The distribution of moving groups in the solar neighborhood has been used to constrain dynamical properties of the Milky Way for decades. The kinematic bimodality between the main…
Exponential galaxy discs as the quasi-stationary distribution in a Markov chain model simulating stellar scattering
Jian Wu, Curtis Struck, Bruce G. Elmegreen +1
Previous models have shown that stochastic scattering of stars in a two-dimensional galaxy disc can generate a time-independent surface density distribution that is an exponential…
The Non-Axisymmetric Influence: Radius and Angle-Dependent Trends in a Barred Galaxy
Carrie Filion, Rachel L. McClure, Martin D. Weinberg +2
Many disc galaxies host galactic bars, which exert time-dependent, non-axisymmetric forces that can alter the orbits of stars. There should be both angle and radius-dependence in t…