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Absolute V-band magnitudes and mass-to-light ratios of Galactic globular clusters
DOI: 10.1017/pasa.2020.38 Bibcode: 2020PASA...37...46B

Hilker, M.; Baumgardt, H.; Sollima, A.

We have used Hubble Space Telescope and ground-based photometry to determine total V-band magnitudes and mass-to-light ratios of more than 150 Galactic globular clusters. We do this by summing up the magnitudes of their individual member stars, using colour-magnitude information, Gaia DR2 proper motions, and radial velocities to distinguish cluste…

2020 Publications of the Astronomical Society of Australia
Gaia eHST 54
Galaxy spin direction distribution in HST and SDSS show similar large-scale asymmetry
DOI: 10.1017/pasa.2020.46 Bibcode: 2020PASA...37...53S

Shamir, Lior

Several recent observations using large data sets of galaxies showed non-random distribution of the spin directions of spiral galaxies, even when the galaxies are too far from each other to have gravitational interaction. Here, a data set of$\sim8.7\cdot10^3$spiral galaxies imaged byHubble Space Telescope(HST) is used to test and profile a possibl…

2020 Publications of the Astronomical Society of Australia
eHST 18
ASKAP reveals giant radio halos in two merging SPT galaxy clusters
DOI: 10.1017/pasa.2020.34 Bibcode: 2020PASA...37...40W

Johnston-Hollitt, Melanie; Akamatsu, Hiroki; Hodgson, Torrance +4 more

Early science observations from the Australian Square Kilometre Array Pathfinder (ASKAP) have revealed clear signals of diffuse radio emission associated with two clusters detected by the South Pole Telescope via their Sunyaev Zel'dovich signal: SPT CLJ0553-3342 (MACS J0553.4-3342) and SPT CLJ0638-5358 (Abell S0592) are both high-mass lensing clus…

2020 Publications of the Astronomical Society of Australia
eHST 14