activity
20172026
most citedA ~600 pc view of the strongly-lensed, massive main sequence galaxy J0901: a baryon-dominated, thick turbulent rotating disk with a clumpy cold gas ring at z = 2.259

22 citations · 123 across the 30 of their papers we have counts for

collaborators
Showing 2020Show all

4 papers · 1 filter

astro-ph.GA2020

Extreme kinematic misalignment in IllustrisTNG galaxies: the origin, structure and internal dynamics of galaxies with a large-scale counterrotation

Sergey Khoperskov, Igor Zinchenko, Branislav Avramov +9

Modern galaxy formation theory suggests that the misalignment between stellar and gaseous components usually results from an external gas accretion and/or interaction with other ga…

astro-ph.GA2020

The stellar halos of ETGs in the IllustrisTNG simulations: II. Accretion, merger history, and dark halo connection

C. Pulsoni, O. Gerhard, M. Arnaboldi +5

Stellar halos in early-type galaxies (ETGs) are shaped by their accretion and merger histories. We use a sample of 1114 ETGs in the TNG100 simulation with stellar masses $10^{10.3}…

astro-ph.GA2020★ 19 cited

The halo of M105 and its group environment as traced by planetary nebula populations: I. Wide-field photometric survey of planetary nebulae in the Leo I group

J. Hartke, M. Arnaboldi, O. Gerhard +6

M105 (NGC 3379) is an early-type galaxy in the Leo I group. This group is the nearest group that contains all main galaxy types and can thus be used as a benchmark to study the pro…

astro-ph.GA2020

The stellar halos of ETGs in the IllustrisTNG simulations: the photometric and kinematic diversity of galaxies at large radii

C. Pulsoni, O. Gerhard, M. Arnaboldi +4

We characterize the photometric and kinematic properties of simulated early-type galaxy (ETG) stellar halos, and compare them to observations. We select a sample of ~1200 ETGs in t…