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 Milky Way's magnetic field is critical for shaping the structure and evolution of the galaxy, regulating star formation, and transporting cosmic rays. Understanding the interaction between the magnetic field and atomic HI gas is key to unraveling the galaxy's dynamics and evolution.

Student intake

Open for Honours students

People

Mapping azimuthal variations in metals across cosmic time

Student intake

Open for PhD students

People

With this project we will be using the newly automated ANU 2.3m telescope and the powerful WiFeS optical spectrograph to perform a time-series measurement of luminous active galaxies (AGN) using the technique of Quasar Reverberation Mapping.

Student intake

Open for Bachelor, Honours, PhD students

People

Student intake

Open for Honours, PhD students

In this project, the student would study both the spectral and structural properties of the thermal electron density and magnetic fields in the ionised gas phase of the Milky Way.

Student intake

Open for Bachelor, Honours, PhD students

People

In this project we will be able to investigate the environmental effect on star formation and galaxy evolution in individual galaxies falling into the cluster through radio observations of active galactic nuclei (AGN).

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

New 3-D technology to explore the Universe, after winning a $30 million Centre of Excellence from the Australian Research Council (ARC).

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Astronomers have solved a mystery over small, unusually hot blue stars, 10 times hotter than our Sun, that are found in the middle of dense star clusters.

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The universe's benchmark explosions are much more varied than expected.

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Astronomers have glimpsed a far off and ancient star exploding, not once, but four times.

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