Click on images to obtain high resolution files.
|
Mpeg
file showing
a rotating data section from the 2dF Galaxy Redshift Survey. |
|
The 2dFGRS data cone, showing the
distribution of galaxies. High resolution file is much clearer than the
thumbnail. Credit: 2dfGRS. |
|
Image of the Cosmic Microwave Background,
emitted 380,000 years after the Big Bang. Credit: WMAP Science Team /
NASA |
|
7,000 stars and the Milky Way, Credit: Knut
Lundmark, Copyright: Lund
Observatory,
|
|
Computer simulation of matter forming into
galaxies. The first picture is the furthest point back in time,
redshift 3, the second picture is a mid-point and the third picture
simulates the structure at redshift zero, the present day. Higher
resolution images are available behind each link, but are not huge. A
single bigger simulation is available here.
Copyright Virgo
Consortium. |
|
The galaxy map produced by the 2dF Galaxy
Redshift Survey. Each dot is a
galaxy. Earth is at the centre of the 'bow-tie'. Red areas are more
dense,
blue areas less dense. Image by Paul Bourke, Swinburne University
Centre for
Astrophysics and Supercomputing. |
|
Siding Spring Observatory showing the AAT
(foreground) and the Schmidt telescope (background). Copyright
Anglo-Australian Observatory. Photo by David Malin. |
|
The 2dF instrument mounted on the
Anglo-Australian Telescope. Credit: Anglo-Australian Observatory
|
|
The 3.9-m Anglo-Australian Telescope.
Photo: Shaun Amy |
|
2dF Data Fly-through movie
A visualisation of a trip through the Universe based
on data from the 2dF Galaxy Redshift Survey. The galaxies are shown in
their
actual positions in space. The fly-through is a collaborative project
of
Swinburne University of Technology's Centre for Astrophysics and
Supercomputing
and the Anglo-Australian Observatory.
2dF movie version1
and version2.
|
|
2dFGRS cone plot. The distribution of
galaxies revealed by the 2dFGRS. Each dot is galaxy. The Earth is
at the centre of the 'bow-tie'. The wedges are views stretching out of
our Galaxy towards the North and South Galactic Poles.
|
|