Abell 2142 radio images
收藏B2FIND2026-03-19 收录
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https://b2find.eudat.eu/dataset/e4741199-f6b2-5005-9a9e-17b0cbe29ffb
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Tailed radio galaxies are shaped by ram pressure owing to the high-velocity motion of their host through the intracluster medium (ICM). Recent works have reported on the...
