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・ Abell 1413
・ Abell 1689
・ Abell 1795
・ Abell 1835
・ Abell 1835 IR1916
・ Abell 1991
・ Abell 2029
・ Abell 2061
・ Abell 2065
・ Abell 2067
・ Abell 2142
・ Abell 2147
・ Abell 2162
・ Abell 2163
・ Abell 2199
Abell 2218
・ Abell 222
・ Abell 223
・ Abell 2256
・ Abell 2261
・ Abell 2390
・ Abell 262
・ Abell 2667
・ Abell 2744
・ Abell 2744 Y1
・ Abell 31
・ Abell 3266
・ Abell 33
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Abell 2218 : ウィキペディア英語版
Abell 2218

Abell 2218 is a cluster of galaxies about 2 billion light-years away in the constellation Draco.
Acting as a powerful lens, it magnifies and distorts all galaxies lying behind the cluster core into long arcs. The lensed galaxies are all stretched along the cluster's center and some of them are multiply imaged. Those multiple images usually appear as a pair of images with a third — generally fainter — counter image, as is the case for the very distant object. The lensed galaxies are particularly numerous, as we are looking in between two mass clumps, in a saddle region where the magnification is quite large.
==Gravitational lensing==
Abell 2218 was used as a gravitational lens to discover the most distant known object in the universe as of 2004. The object, a galaxy some 13 billion years old, is seen from Earth as it would have been just 750 million years after the Big Bang.〔(MSNBC: "Galaxy ranks as most distant object in cosmos" )〕
The color of the lensed galaxies is a function of their distances and types. The orange arc is an elliptical galaxy at moderate redshift (z=0.7). The blue arcs are star-forming galaxies at intermediate redshift (z=1-2.5). The encircled very red pair is the newly discovered star-forming galaxy at about redshift 7.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
ウィキペディアで「Abell 2218」の詳細全文を読む



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