Chris Flynn : Tuorla Observatory

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Galaxy clusters

Galaxies almost always come in groups of a few (such as the Local Group) to as many as a few thousand (e.g. the Virgo cluster). These mass concentrations thus contain tracer particles (the galaxies themselves) which can be used to reconstruct the mass distribution of the total system). A dark matter problem emerges in these studies which is even more serious than the one for the Galaxy (i.e. individual galaxies) mentioned above. This ROSAT image (right) of the Virgo cluster of galaxies reveals a hot X-ray emitting plasma or gas with a temperature of 10-100 million degrees pervading the cluster. False colors have been used to represent the intensity of X-ray emission. The large area of X-ray emission, just below and left of center, is about 1 million light-years across. The giant elliptical galaxy M87(see optical image), the biggest member of the cluster, is centered in that area while other cluster members are scattered around it. By adding up the amount of X-ray emitting gas astronomers have found that its total mass is up to 5 times the total mass of the cluster galaxies themselves - yet all this matter still does not produce nearly enough gravity to keep the cluster from flying apart! What is the unseen mass?
 
Einstein showed that massive objects can bend the path of lightbeams, and if they are compact enough focus the light like a lens does in a telescope. The image shows how distant (background galaxies) have been magnified and distorted by the matter distribution in a foreground cluster of galaxies. The foreground galaxies are mostly yellow, and the background ones blueish.

Studies of images like this show that there is a lot more matter in this cluster of galaxies than just that in the visible galaxies and gas. 


 
clusters in optical and X ray
 
X-ray and Optical  images of the galaxy cluster in the constellation Virgo. The optical image shows the visible galaxies in the cluster (right), while the X-ray image displays the hot gas which resides between the galaxies (left).   Source : GSFC
 
 
 
 
 
lenses
Lensed galaxies appear blue in this image of a nearby cluster. The yellow galaxies are the ones acting as the lenses.   Source : HST



 








For further information:  

Chris Flynn
Tuorla Observatory
Väisäläntie 20
FIN-21500 Piikkiö
Finland

Tel: +358 (0)2 2744244
Fax: +358 (0)2 2433767
email: cflynn@astro.utu.fi





Antares

Research supported by the ANTARES program of the Academy of Finland