Theoretical astrophysics

Theoretical astrophysics

The Theorectical Astrophysics research program explores the areas of compact stars, radiation processes and transfer mechanisms in accretion flows on to highly magnetic compact stars, modelling of accretion disks, modelling of stars and magnetic atmospheres, cataclysmic variable binaries, and searching for the progenitors of type Ia supernovae.

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About

The Theorectical Astrophysics research program explores the areas of: 

  • compact stars, such as white dwarfs, neutron stars (pulsars and magnetars ) and black holes
  • radiation processes and transfer mechanisms in accretion flows on to highly magnetic compact stars
  • modelling of accretion disks
  • modelling of stars and magnetic atmospheres
  • cataclysmic variable binaries
  • searching for the progenitors of type Ia supernovae.

Projects

The discovery of strong 17 per cent circular polarisation in the IR in the Orion OMC-1 star forming region has provided a new impetus to the view that the homochirality of natural amino-acids seen in biological systems on Earth may have been triggered by asymmetric photolysis of biogenic amino acids in space.

Student intake

Open for PhD students

Status

Potential

People

About 50 percent of stars in our Galaxy occur in binary systems. The orbits of such systems evolve with time due to a variety of mechanisms involving mass and angular momentum loss.

Student intake

Open for PhD students

Status

Potential

People

It is proposed that the student presents a review of the theory of black hole formation, and a critical evaluation of the arguments used to deduce their existence in the universe.

Student intake

Open for Honours, Masters, PhD students

Status

Potential

People

Astronomers are often faced with the problem of constructing models for systems which are not fully constrained by observational data.

Student intake

Open for PhD students

Status

Potential

People

The polarised radiative transfer equations consist of four coupled first order differential equations in the four Stokes parameters which describe the radiation field.

Student intake

Open for PhD students

Status

Potential

People

Echelle spectroscopy (here Hamilton echelle at the Lick Observatory 3m telescope) of short period evolved binaries is the key to understanding the origin of cataclymic variables.

Student intake

Open for PhD students

Status

Potential

People

Members

Collaborator

No photo provided

Honorary Associate Professor

Convenor

Lilia Ferrario

MSI Director
Professor

Researcher

Dayal Wickramasinghe

Emeritus Professor

Student