… In Figure 3, we show an example of these fits comparing low and high ions. Note that while
we only show Si ii λ1260 in this figure, the fit of the Si ii is actually based on three transitions …

… kinematic extent of the gas that fuels galaxies … gas from the Figuring Out Gas & Galaxies in
Enzo (FOGGIE) project and link these maps back to physical and spatial properties of the gas. …

… The galaxies we analyze in this paper are from the Figuring Out Gas & Galaxies in Enzo (FOGGIE)
simulation suite. The FOGGIE simulations were first introduced in Peeples et al. (2019…

… gas motions. Using simulations of low-redshift, ∼L* galaxies from the Figuring Out Gas &
Galaxies In Enzo (FOGGIE) project that are optimized to resolve low-density gas, we show …

… In Figure 2, we show the volume-weighted distribution of densities and velocities (left
panel) and the temperature-coded ram pressure profile (right panel) of the CGM gas inside …

… variations in the gas density. The CGM in the FOGGIE simulations has significant density
variations (eg, see Figure 4) that are not our main focus in this work, so we normalize them out. …

… In §5.1 and Figure 6 we examine how the orientations of the angular momenta (⃗L) of the
cold gas and dark matter in each of the FOGGIE halos: (1) evolve in time, (2) vary as a function …

… We can see it again in an expression like the noble gases, where the word noble-regardless
of its origins and the reasons for its choice-now has a fairly precise chemical meaning that …

… ABSTRACT Gas-phase metallicity gradients are a crucial … gas-phase metallicity will be
needed to relate trends in upcoming high-z JWST observations with the underlying physics of gas …

… The challenge in figuring out how climate change will influence soil properties and
processes is in working out the complex interactions that take place as conditions change. …