YOU ARE HERE: Home > News & Press > News archive > News 2006 > RAS PN 06/20 (NAM13): Giant filaments give rare insight into galaxy cluster evolution

I want information on:

Information for:


RAS PN 06/20 (NAM13): Giant filaments give rare insight into galaxy cluster evolution

Last Updated on Sunday, 01 December 2013 20:49
Published on Wednesday, 05 April 2006 00:00
A new image of the centre of a cluster of galaxies has revealed massive filamentary structures that give a rare insight into the evolution of galaxy clusters.
“The star forming regions in the cluster that we’d observed previously were just the tip of the iceberg.  We’ve now observed filaments of gas streaming out from these regions that are approximately 490 thousand light years across. The gaseous trails mark the path of galaxies travelling at high speed through the cluster. The origin of these unique features is still a matter for debate, but we think the combined action of tidal forces among galaxies in the cluster and of ram-pressure by the ambient medium caused the galaxies to fragment and blast out the ionized gas,” said Dr Luca Cortese, who is presenting the results at the Royal Astronomical Society’s National Astronomy Meeting on 5th April. 

An international team, lead by Dr Cortese, studied the physical properties of a compact group that is falling towards the centre of a cluster of galaxies known as Abell1367 at a rate of 1700 km/s.  The group, which was discovered in 2002, has the highest density of star forming objects ever observed in local clusters. It contains two giant galaxies, at least ten dwarf galaxies or extragalactic clouds of gas and over a billion solar masses of diffuse gas filaments.   

Scientists believe that clusters of galaxies are formed from the accretion of compact groups like the one observed in Abell1367. Formation of clusters of galaxies peaked 5 billion years ago. Now the rate is at least three times lower and it will slow dramatically due to the effects of the acceleration of the Universe. The Abell1367 group is particularly important as it is only 300 million light years from Earth – ‘local’ in terms of the Universe – and so the scientists can see the processes at work in unprecedented detail.  Dr Cortese explains, “The physical processes seen here are typical of young clusters, found far away in space and a long time ago.  To really understand what’s going on, we need a close up view. This is the first time we have found an example of a galaxy group mid-way through its transformation that is close enough for us to have a really good look at the structures surrounding the galaxies.”

The results suggest that at least part of the changes to the structure of cluster galaxies that took place in earlier epochs happened very differently to ones observed in today’s clusters. In today’s clusters of galaxies, the galaxies are travelling faster than in the infalling groups, which means that gravitational interactions between galaxies happen much faster.
The study was carried out using the Italian National Telescope Galileo in La Palma in April 2004 and February 2006. 
The results of this study are accepted for publication on Astronomy and Astrophysics

This study has been undertaken in collaboration with:

Prof. Giuseppe Gavazzi – Universita’ degli Studi di Milano-Bicocca, Italy
Dott. Alessandro Boselli – Laboratoire d’Astrophysique de Marseille, France
Dott. Paolo Franzetti – IASF-INAF Milano, Italy
Prof. Robert Kennicutt – Institute of Astronomy, Cambridge, UK
Dott. Karen O’Neil – NRAO, USA
Dott. Shoko Sakai – UCLA, USA
Telescopio Nazionale Galileo (TNG)

The Telescopio Nazionale Galileo (TNG), with a primary mirror of 3.58m, is the national facility of the Italian astronomical community.  It is located at Roque de Los Muchachos Observatory on La Palma, Canary Islands, and is operated by the Italian National Institute of Astrophysics (INAF).

TNG is equipped with 5 instruments which are permanently operating on its foci and offer a large variety of observing modes covering the optical and near infrared wavelength ranges and spanning from broad band imaging to high resolution spectroscopy.

For more information, visit:

Royal Astronomical Society’s National Astronomy Meeting
The 2006 RAS National Astronomy Meeting is hosted by the University of Leicester. It is sponsored by the Royal Astronomical Society, the UK Particle Physics and Astronomy Research Council (PPARC), the University of Leicester and the National Space Centre, Leicester.

Dr Luca Cortese
School of Physics and Astronomy
Cardiff University
5, The Parade
Cardiff CF24 3YB
Tel. +44 (0)2920876992
Fax. +44 (0)2920874056
This email address is being protected from spambots. You need JavaScript enabled to view it.

From Wednesday 5th until Thursday 6th April, Dr Cortese can be contacted via the NAM press office (see above).

For images of the filament structures, see: