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5 papers · 2 filters
The AGORA High-Resolution Galaxy Simulations Comparison Project. II: Isolated Disk Test
Ji-hoon Kim, Oscar Agertz, Romain Teyssier +40
Using an isolated Milky Way-mass galaxy simulation, we compare results from 9 state-of-the-art gravito-hydrodynamics codes widely used in the numerical community. We utilize the in…
Incidence of WISE-Selected Obscured AGNs in Major Mergers and Interactions from the SDSS
Madalyn E. Weston, Daniel H. McIntosh, Mark Brodwin +4
We use the Wide-field Infrared Survey Explorer (WISE) and the Sloan Digital Sky Survey (SDSS) to confirm a connection between dust-obscured active galactic nuclei (AGNs) and galaxy…
Galaxy Simulation with Dust Formation and Destruction
Shohei Aoyama, Kuan-Chou Hou, Ikkoh Shimizu +4
We perform smoothed particle hydrodynamics (SPH) simulations of an isolated galaxy with a new treatment for dust formation and destruction. To this aim, we treat dust and metal pro…
The Ultraviolet and Infrared Star Formation Rates of Compact Group Galaxies: An Expanded Sample
Laura Lenkic, Panayiotis Tzanavaris, Sarah Gallagher +8
Compact groups of galaxies provide insight into the role of low-mass, dense environments in galaxy evolution because the low velocity dispersions and close proximity of galaxy memb…
Disc colours in field and cluster spiral galaxies at 0.5 < z < 0.8
Nicolas Cantale, Pascale Jablonka, Frederic Courbin +9
We present a detailed study of the colours in late-type galaxy discs for ten of the EDisCS galaxy clusters with 0.5 < z < 0.8. Our cluster sample contains 172 spiral galaxies, and…