Measuring reliable stellar abundances towards crowded regions using MUSE
With the rapid development of stellar spectroscopy in the past decade, many stellar spectroscopic surveys, for example LAMOST, GALAH and APOGEE, combined with the astrometric information of Gaia have played a pivotal role in explaining the chemo-dynamic evolution of the Milky Way. By extracting the elemental abundances and ages of millions of stars from the …
Australian-based astronomers to take a deep dive into the cosmos with time awarded on one of ESO’s most powerful instruments
Two teams of astronomers led by The University of Sydney and by The University of Western Australia node of the International Centre for Radio Astronomy Research (ICRAR/UWA) have recently each been awarded substantial amounts of observing time on one of the most in-demand instruments at the European Southern Observatory (ESO) – the Multi Unit Spectroscopic …
A FLASH combination: ASKAP and MUSE sniff out gas around galaxies
The timescales in which star-forming galaxies deplete their gas is found to be short relative to the age of the Universe. This points to the conclusion that galaxies must have a way to replenish their gas reservoirs and indeed, early cosmological simulations reveal cold gas being channeled along dark matter filaments. At the same time, …
Detailed cross-section of another galaxy reveals surprising similarities to our home
The first detailed cross-section of a galaxy broadly similar to the Milky Way, published today, reveals that our galaxy evolved gradually, instead of being the result of a violent mash-up. The finding throws the origin story of our home into doubt. The first detailed cross-section of a galaxy broadly similar to the Milky Way, published …