activity
19952026
most citedFormation of Hard Power-laws in the Energetic Particle Spectra Resulting from Relativistic Magnetic Reconnection

461 citations · 7.4k across the 158 of their papers we have counts for

collaborators
Showing 2018 · astro-ph.GAShow all

6 papers · 2 filters

astro-ph.GA2018★ 47 cited

Early-type galaxy density profiles from IllustrisTNG: I. Galaxy correlations and the impact of baryons

Yunchong Wang, Mark Vogelsberger, Dandan Xu +10

We explore the isothermal total density profiles of early-type galaxies (ETGs) in the IllustrisTNG simulation. For the selected 559 ETGs at with stellar mass $10^{10.7}\mat…

astro-ph.GA2018★ 76 cited

Star cluster formation in cosmological simulations. III. Dynamical and chemical evolution

Hui Li, Oleg Y. Gnedin

In previous papers of this series, we developed a new algorithm for modeling the formation of star clusters in galaxy formation simulations. Here we investigate how dissolution of…

astro-ph.GA2018★ 19 cited

Structure and stability of high-redshift galaxies in cosmological simulations

Xi Meng, Oleg Y. Gnedin, Hui Li

We investigate the structure of galaxies formed in a suite of high-resolution cosmological simulations. Consistent with observations of high-redshift galaxies, our simulated galaxi…

astro-ph.GA2018★ 44 cited

The star clusters that make black hole binaries across cosmic time

Nick Choksi, Marta Volonteri, Monica Colpi +2

We explore the properties of dense star clusters that are likely to be the nurseries of stellar black holes pairing in close binaries. We combine a cosmological model of globular c…

astro-ph.GA2018★ 24 cited

Nuclear Star Clusters in Cosmological Simulations

Gillen Brown, Oleg Y. Gnedin, Hui Li

We investigate the possible connection between the most massive globular clusters, such as Cen and M54, and nuclear star clusters of dwarf galaxies that exhibit similar spreads…

astro-ph.GA2018★ 115 cited

Formation of Globular Cluster Systems: From Dwarf Galaxies to Giants

Nick Choksi, Oleg Gnedin, Hui Li

Globular cluster (GC) systems around galaxies of a vast mass range show remarkably simple scaling relations. The combined mass of all GCs is a constant fraction of the total galaxy…