Cosmos

Structure and evolution of the Cosmos

Explores the vast complexities of the cosmos, focusing on the formation and interaction of galaxies, the early universe, dark matter, and cosmic expansion, contributing to groundbreaking discoveries like the accelerating expansion of the universe, a phenomenon pivotal to our understanding of cosmic evolution.

About

On the largest and most distant scales, astrophysicists and cosmologists at RSAA study many types of distant galaxies, investigate the nature of the early universe, and measure the expansion of space itself. Areas of study in these fields include:

  • understanding how galaxies form and interact with each other and their environments
  • observing how interactions between galaxies affect their development
  • the effects of internal processes, such as star formation and central supermassive black holes, on the growth of a galaxy
  • the role and nature of dark matter in the formation of structure in the universe
  • measuring the rate of acceleration of the expansion of the universe and understanding the implications for cosmological models
  • modelling and observing enigmatic phenomena such as gamma ray bursts, supernovae and other transients to understand the physical processes that cause them.

Research led by cosmologists at ANU led to the discovery that the Universe is expanding at an ever-increasing rate; work for which the 2011 Nobel Prize in Physics was awarded. RSAA astronomers continue to investigate what this means for theoretical models of the Universe, to understand the role of dark energy or the cosmological constant that drives this accelearation. They are also improving measurements of distance to the exploding stars, or supernovae, that are used as beacons in mapping the expansion rate to refine the results that constrain these models. One of the major goals for the SkyMapper Telescope's Southern Sky Survey is to discover tens of thousands of new supernova occurring in distant galaxies. This will significantly increase the sample of observed events and enable astronomers to make detailed follow-up observations to help improve understanding of the physical processes that occur during these stellar explosions.

Projects

The main aim of this project is to parallelise an existing Fortran program to take advantage of the parallel processing environment of the supercomputer raijin, located on the ANU campus.

This project will study red spirals in detail, and aim to understand what levels of star formation persist and for how long. We will use optical and infrared data to measure current rates of star formation and find out what we have been missing due to dust extinction.

This projects aim to understand new methods for estimating the stellar masses of distant galaxies using imaging from the James Webb Space Telescope.

Student intake

Open for Bachelor, Honours students

People

Our team is looking for enthusiastic Honours, Masters and PhD students with a strong background in Maths, Physics, or Computer Science who want to work on some of the most important questions currently discussed in near-field cosmology community.

Student intake

Open for Honours, PhD students

People

This project is intended to search for the magnetic field signature of the Magellanic halo.

Student intake

Open for Bachelor, Honours, PhD students

People

The goal of this project is to build a software pipeline that can take simulations of galactic winds, such as the one shown in the figure, and make simulated observational images from them that can be compared directly to telescopic data.

Student intake

Open for Honours students

People

Members

Academic

Christoph Federrath

Associate Director HDR
Former ARC Future and Stromlo Fellow
Research School of Astronomy and Astrophysics

Faculty

Christoph Federrath

Associate Director HDR
Former ARC Future and Stromlo Fellow
Research School of Astronomy and Astrophysics

News

The Australian Research Council has announced that the Research School of Astronomy and Astrophysics has won funding for two prestigious Future Fellowships.

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By identifying a second galactic wind in one compact group, the results of Frédéric's research may help astronomers better understand the formation of galactic outflows.

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The group have been studying these supernovae for several years and having analysed their data, have come to the surprising conclusion that far from slowing down, the rate of expansion of the universe is actually speeding up.

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A PhD student at the ANU Research School of Astronomy and Astrophysics, Catherine Farage, is studying massive ellipticals in galaxy clusters, to look for clues that could help to explain the mechanisms behind the formation of large galaxies.

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SkyMapper will be the first survey telescope to create a detailed digital map of the southern skies

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