Strong ram-pressure stripping and widespread star formation in the high-velocity system towards the center of the Perseus cluster
I present spectroscopic imaging of the high-velocity system (HVS) towards the central cD galaxy (NGC 1275) in the Perseus Cluster at a high spectral resolution for the first time. Previous observation suggests that the HVS is a highly inclined dusty and gas-rich galaxy moving towards the center of N...
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| Language: | English |
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The University of Hong Kong (Pokfulam, Hong Kong)
2015
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| Online Access: | http://hdl.handle.net/10722/211150 |