papers

Publications (7)

astro-ph.GA2026

The initial conditions and initial mass functions of Alpha Persei, Pleiades and Praesepe

L. Hobart, H. Baumgardt, S. Sweet

We have determined the initial mass function (IMF) and structural properties of the open clusters Alpha Persei, Pleiades and Praesepe using Gaia DR3 astrometry and photometry. Clus…

astro-ph.GA2019

The SAMI Galaxy Survey: First detection of a transition in spin orientation with respect to cosmic filaments in the stellar kinematics of galaxies

C. Welker, J. Bland-Hawthorn, J. Van de Sande +16

We present the first detection of mass dependent galactic spin alignments with local cosmic filaments with over 2 sigma confidence using IFS kinematics. The 3D network of cosmic fi…

astro-ph.GA2019

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.GA2018

The SAMI Galaxy Survey: gas content and interaction as the drivers of kinematic asymmetry

J. V. Bloom, S. M. Croom, J. J. Bryant +21

In order to determine the causes of kinematic asymmetry in the H gas in the SAMI Galaxy Survey sample, we investigate the comparative influences of environment and intrinsic pr…

astro-ph.GA2017

The SAMI Galaxy Survey: The cluster redshift survey, target selection and cluster properties

M. S. Owers, J. T. Allen, I. Baldry +40

We describe the selection of galaxies targeted in eight low redshift clusters (APMCC0917, A168, A4038, EDCC442, A3880, A2399, A119 and A85; ) as part of the Sydn…

astro-ph.GA2022

The physical connection between central stellar surface density and stellar spin in SAMI and MaNGA nearby galaxies

L. Cortese, A. Fraser-McKelvie, J. Woo +8

The stellar surface density within the inner 1 kpc () has become a popular tool for understanding the growth of galaxies and its connection with the quenching of star forma…