activity
20032026
most citedDancing in the dark: galactic properties trace spin swings along the cosmic web

888 citations · 7.3k across the 106 of their papers we have counts for

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Showing 2023Show all

6 papers · 1 filter

astro-ph.GA2023★ 17 cited

2D chemical evolution models II. Effects of multiple spiral arm patterns on O, Eu, Fe and Ba abundance gradients

E. Spitoni, G. Cescutti, A. Recio-Blanco +7

According to observations and numerical simulations, the Milky Way could exhibit several spiral arm modes with multiple pattern speeds, wherein the slower patterns are located at l…

astro-ph.GA2023

The formation of cores in galaxies across cosmic time -- the existence of cores is not in tension with the LCDM paradigm

R. A. Jackson, S. Kaviraj, S. K. Yi +9

The `core-cusp' problem is considered a key challenge to the LCDM paradigm. Halos in dark matter only simulations exhibit `cuspy' profiles, where density continuously increases tow…

astro-ph.GA2023

Emergence and cosmic evolution of the Kennicutt-Schmidt relation driven by interstellar turbulence

Katarina Kraljic, Florent Renaud, Yohan Dubois +12

The scaling relations between the gas content and star formation rate of galaxies provide useful insights into processes governing their formation and evolution. We investigate the…

astro-ph.GA2023★ 3 cited

On the Significance of the Thick Disks of Disk Galaxies

Sukyoung K. Yi, J. K. Jang, Julien Devriendt +8

Thick disks are a prevalent feature observed in numerous disk galaxies including our own Milky Way. Their significance has been reported to vary widely, ranging from a few to 100%…

astro-ph.GA2023★ 17 cited

Analytic solution of Chemical Evolution Models with Type Ia SNe

P. A. Palicio, E. Spitoni, A. Recio-Blanco +3

Context: In the last years, a significant number of works have focused on finding analytic solutions for the chemical enrichment models of galactic systems, including the Milky Way…

astro-ph.CO2023

LyAl-Net: A high-efficiency Lyman- forest simulation with a neural network

Chotipan Boonkongkird, Guilhem Lavaux, Sebastien Peirani +3

The inference of cosmological quantities requires accurate and large hydrodynamical cosmological simulations. Unfortunately, their computational time can take millions of CPU hours…