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・ Abell 2390
・ Abell 262
・ Abell 2667
・ Abell 2744
・ Abell 2744 Y1
・ Abell 31
・ Abell 3266
・ Abell 33
・ Abell 36
・ Abell 370
・ Abell 383
・ Abell 39
・ Abell 400
・ Abell 478
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Abell 665
・ Abell 671
・ Abell 7
・ Abell 70
・ Abell 754
・ Abell 78
・ Abell 907
・ Abell Catalog of Planetary Nebulae
・ Abell catalogue
・ Abell Farmhouse and Barn
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・ Abell House (Leonardtown, Maryland)
・ Abell S1077
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Abell 665 : ウィキペディア英語版
Abell 665

Abell 665 is a galaxy cluster in the Abell catalogue in the constellation Ursa Major. It is also known as the only cluster in his 1989 catalog to receive Abell's highest richness class of 5. This means that it contains ''at least'' 300 galaxies in the magnitude range of m3 to m3+2, where m3 is the magnitude of the 3rd brightest member of the cluster. The clusters in all other richness classes contain less than 300 such galaxies. Abell 665's combination of high brightness and large distance, made it an excellent candidate along with 37 other clusters to help determine the Hubble constant using the Sunyaev–Zel'dovich effect in 2006.〔
Member velocity, cluster velocity dispersion, and X-ray data suggest that Abell 665 is composed of 2 similar-mass clusters which are at or very close to core crossing, give or take ≲ 0.5 Gyr.
==See also==

* List of Abell clusters

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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