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・ Cangetta furvitermen
・ Cangetta haematera
・ Cangetta hartoghialis
・ Cangetta homoperalis
・ Cangetta micralis
・ Cangetta murinalis
・ Cangetta primulina
・ Cangey
・ Caner Erkin
・ Caner Koca
・ Caner Osmanpaşa
・ Caner Pekşen
・ Caner Topaloğlu
・ Caner Çolak
・ Canertinib
Canes II Group
・ Canes Venatici
・ Canes Venatici (Chinese astronomy)
・ Canes Venatici Dwarf Galaxy
・ Canes Venatici I (dwarf galaxy)
・ Canes Venatici II (dwarf galaxy)
・ Canesadooharie
・ Canesadooharie River
・ Canesta
・ Canestrato
・ Canestrelli
・ Canestrini's goby
・ Canestru
・ Canet
・ Canet d'Adri


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Canes II Group : ウィキペディア英語版
Canes II Group

The Canes II Group or Canes Venatici II Group (CVn II Group) is a group of galaxies about 26.1 million light-years away from Earth. The group resides in the Local Supercluster.〔G. De Vaucouleurs, 1975. ''Nearby Groups of Galaxies'', ch. 5. the nearer groups within 10 megaparsecs. Published in "Galaxies and the Universe," ed. by A. Sandage, M. Sandage and J. Kristian〕 The largest galaxy within the cluster is M106 (NGC 4258), which is a barred spiral galaxy.
==Galaxies in the Cluster==
Canes II is directly behind Canes I, which makes it difficult to show which galaxy belongs in which cluster. It is generally accepted that the following galaxies belong in Canes II;

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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