McKeown et al., available on arXiv Abstract: We use FIRE-2 zoom cosmological simulations of Milky Way size galaxy halos to calculate astrophysical J-factors for dark …
Patel et al., available on arXiv Abstract: We investigate stellar elemental abundance patterns at z = 0 in 8 low-mass (M_* = 10^6 – 10^9 …
Chan et al., available on arXiv Abstract: Cosmic rays (CRs) are an important component in the interstellar medium (ISM), but their effect on the dynamics …
Cunningham et al., available on arXiv Abstract: In the era of large-scale spectroscopic surveys in the Local Group (LG), we can explore using chemical abundances …
Hopkins et al., available on arXiv Abstract: We present the first simulations evolving resolved spectra of cosmic rays (CRs) from MeV-TeV energies (including electrons, positrons, …
Kado-Fong et al., available on arXiv Abstract: Extended, old, and round stellar halos appear to be ubiquitous around high-mass dwarf galaxies (10^8.5 < Mstar/Msun < …
Stern et al., available on arXiv Abstract: Recent searches for the hosts of high-redshift (z~4) damped Ly-alpha absorbers (DLAs) have detected bright galaxies at distances …
Trapp et al., available on arXiv Abstract: Observations indicate that a continuous supply of gas is needed to maintain observed star formation rates in large, …
Panithanpaisal et al., available on arXiv Abstract: Stellar streams record the accretion history of their host galaxy. We present a set of simulated streams from …
Nikakhtar et al., available on arXiv Abstract: The standard picture of galaxy formation motivates the decomposition of the Milky Way into 3–4 stellar populations with …