K-CLASH: Strangulation and ram pressure stripping in galaxy cluster members at 0.3 < z < 0.6

K-CLASH: Strangulation and ram pressure stripping in galaxy cluster members at 0.3 < z < 0.6

Galaxy clusters have long been theorized to quench the star formation of their members. This study uses integral-field unit observations from the K-band MultiObject Spectrograph (KMOS) – Cluster Lensing And Supernova survey with Hubble (CLASH) survey (K-CLASH) to search for evidence of qu...

Полное описание

Библиографические подробности
Главные авторы:	Vaughan, SP, Tiley, AL, Davies, RL, Prichard, LJ, Croom, SM, Bureau, M, Stott, JP, Bunker, A, Cappellari, M, Ansarinejad, B, Jarvis, MJ
Формат:	Journal article
Язык:	English
Опубликовано:	Oxford University Press 2020

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