activity
20152023
most citedNIHAO X: Reconciling the local galaxy velocity function with Cold Dark Matter via mock HI observations

78 citations · 236 across the 9 of their papers we have counts for

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Showing astro-ph.GAShow all

14 papers · 1 filter

astro-ph.GA2019

Drivers of disc tilting I: Correlations and possible drivers for Milky Way analogues

Samuel W. F. Earp, Victor P. Debattista, Andrea V. Macciò +3

The direction of the spin vectors of disk galaxies change over time. We present the tilting rate of a sample of galaxies in the NIHAO suite of cosmological hydrodynamical simulatio…

astro-ph.GA2019★ 38 cited

Metal-poor stars observed with the automated planet finder telescope. I. Discovery of five carbon-enhanced metal-poor stars from LAMOST

Mohammad K. Mardini, Haining Li, Vinicius M. Placco +6

We report on the discovery of five carbon-enhanced metal-poor (CEMP) stars in the metallicity range of [Fe/H] . These stars were selected from the LAMOST DR3 low-res…

astro-ph.GA2019★ 19 cited

Angular momentum of galaxies and their local analogues with adaptive optics

Sarah M. Sweet, Deanne B. Fisher, Giulia Savorgnan +9

We present stellar specific angular momentum measurements of two galaxies in the KGES sample and 12 DYNAMO analogues of high-redshift galaxies. We com…

astro-ph.GA2019

Size-scaling of clump instabilities in turbulent, feedback regulated disks

Kamran Ali, Danail Obreschkow, Liang Wang +5

We explore the scaling between the size of star-forming clumps and rotational support in massively star-forming galactic disks. The analysis relies on simulations of a clumpy galax…

astro-ph.GA2018

Angular momentum evolution of bulge stars in disc galaxies in NIHAO

Liang Wang, Danail Obreschkow, Claudia del P. Lagos +6

We study the origin of bulge stars and their angular momentum (AM) evolution in 10 spiral galaxies with baryonic masses above M in the NIHAO galaxy formation simul…

astro-ph.GA2018

Spatially-resolved galaxy angular momentum

Sarah M. Sweet, Deanne B. Fisher, Karl Glazebrook +3

The total specific angular momentum j of a galaxy disk is matched with that of its dark matter halo, but the distributions are different, in that there is a lack of both low- and h…