black hole

Black hole phenomena

Explores black hole phenomena, focusing on their nature, roles in galaxies, and impacts such as the formation of active galactic nuclei and galaxy evolution.

About

Black holes are among the most fascinating objects in astrophysics, and it is now thought that many of the most energetic processes in the universe are related, or attributable to, these enigmatic phenomena. Astrophysicists at RSAA study many aspects of the nature of black holes and the roles that they play in galaxies, including:

  • supermassive black holes in galaxies and the formation of active galactic nuclei as material is accreted by the black hole
  • feedback of mass and energy from the nucleus of galaxies as the black hole accretes matter, and how this affects the galaxies, their surroundings, and the way that they grow and develop
  • radio galaxies and the nature of the relativistic jets that are formed in the active galactic nucleus
  • constructing theoretical and computational models of accretion disks around black holes and jets and outflows associated with these phenomena
  • making detailed observations of galaxies, to understand how the central black hole affects their structure and dynamics, and to measure the black hole mass.
  • investigating the nature of the objects that produce highly energetic 'gamma ray bursts' in the distant universe.

Our theoretical astrophysicists develop and run sophisticated computational models to simulate the physical processes at work in these complex systems. They use powerful high-performance computing systems, including the Computational Astrophysics Laboratory (COALA) at RSAA, the ANU Supercomputer Facility (ANUSF), and other supercomputers in Australia.

Projects

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).

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 research project employed the Wide-Field Spectrograph (WiFeS)  to study the extended filaments surrounding a sample of brightest cluster galaxies (BCGs) in massive clusters. Integral-field spectroscopy provides the opportunity to measure the distribution, emission properties, and velocities of the emitting gas across the extent of the galaxies.

Student intake

Open for PhD students

Supermassive black holes in the early Universe are more massive than we can presently explain. We aim to construct their demographics and reveal their origin.

Student intake

Open for Honours, PhD students

People

In this project you will use a new cosmic ray propagation code, CRIPTIC, to model the injection, transport, and final annihilation of positrons in the interstellar medium of the inner Galaxy.

Student intake

Open for Honours, PhD students

People

We aim to build a novel framework to study supermassive black holes via their unique gravitational wave signatures providing a multi-messenger tool to constrain galaxy formation in the early universe.

Student intake

Open for Honours, Master, PhD students

People

  • Dr Lilli (Ling) Sun

News

This is a movie rendered in three dimensions of a supercomputer simulation of a powerful relativistic jet interacting with dense clouds surrounding an active galactic nucleus.

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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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