We study the z= 0 gas kinematics, morphology and angular momentum content of isolated
galaxies in a suite of cosmological zoom-in simulations from the FIRE project spanning M …

We measure, a proxy for galaxy specific stellar angular momentum within one effective
radius, and the ellipticity, ε, for about 2300 galaxies of all morphological types observed with …

We use the TNG100 simulation of the IllustrisTNG project to investigate the stellar specific
angular momenta (j*) of∼ 12 000 central galaxies at z= 0 in a full cosmological context, with …

Dynamical models are crucial for uncovering the internal dynamics of galaxies; however,
most of the results to date assume axisymmetry, which is not representative of a significant …

We use the eagle cosmological hydrodynamic simulation suite to study the specific angular
momentum of galaxies, j, with the aims of (i) investigating the physical causes behind the …

We present the∼ 800 star formation rate maps for the Sydney-AAO Multi-object Integral field
spectrograph (SAMI) Galaxy Survey based on H α emission maps, corrected for dust …

We use eagle to quantify the effect galaxy mergers have on the stellar specific angular
momentum of galaxies, j stars. We split mergers into dry (gas-poor)/wet (gas-rich) …

We present the second major release of data from the Sydney–Australian Astronomical
Observatory Multi-Object Integral Field Spectrograph (SAMI) Galaxy Survey. Data Release …

The formal division of the distance indicators into primary and secondary leads to difficulties
in description of methods which can actually be used in two ways: with, and without the …

The specific angular momenta (j≡ J/M) of stars (j⋆), gas (j gas), baryons as a whole (jb) and
dark matter haloes (jh) contain clues of vital importance about how galaxies form and …