activity
20142026
most citedThe imprint of clump formation at high redshift. I. A disc alpha-abundance dichotomy

111 citations · 685 across the 37 of their papers we have counts for

collaborators
Showing 2019Show all

5 papers · 1 filter

astro-ph.GA2019★ 20 cited

From Peculiar Morphologies to Hubble-type Spirals: The relation between galaxy dynamics and morphology in star-forming galaxies at z~1.5

S. Gillman, A. L. Tiley, A. M. Swinbank +14

We present an analysis of the gas dynamics of star-forming galaxies at z~1.5 using data from the KMOS Galaxy Evolution Survey (KGES). We quantify the morphology of the galaxies usi…

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★ 21 cited

The Dynamics and Distribution of Angular Momentum in HiZELS Star-Forming Galaxies at z = 0.8 - 3.3

S. Gillman, A. M. Swinbank, A. L. Tiley +18

We present adaptive optics assisted integral field spectroscopy of 34 star-forming galaxies at = 0.8-3.3 selected from the HiZELS narrow-band survey. We measure the kinematics…

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.GA2019★ 111 cited

The imprint of clump formation at high redshift. I. A disc alpha-abundance dichotomy

Adam J. Clarke, Victor P. Debattista, David L. Nidever +10

The disc structure of the Milky Way is marked by a chemical dichotomy, with high-alpha and low-alpha abundance sequences, traditionally identified with the geometric thick and thin…