銀河団ガス
1. Intracluster mediumIn astronomy, the intracluster medium (or ICM) is the superheated plasma present at the center of a galaxy cluster. This is gas heated to temperatures of between roughly 10 and 100 megakelvins and consisting mainly of ionised hydrogen and helium, containing most of the baryonic material in the cluster. The ICM strongly emits X-ray radiation.
Read “Intracluster medium” on English Wikipedia
Read “銀河団ガス” on Japanese Wikipedia
Read “Intracluster medium” on DBpedia
Read “Intracluster medium” on English Wikipedia
Read “銀河団ガス” on Japanese Wikipedia
Read “Intracluster medium” on DBpedia
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