K-CLASH: Strangulation and Ram Pressure Stripping in Galaxy Cluster Members at 0.3 < z < 0.6.

Galaxy clusters have long been theorised to quench the star-formation of their members. This study uses integral-field unit observations from the $K$-band Multi-Object Spectrograph (KMOS) - Cluster Lensing And Supernova survey with Hubble (CLASH) survey (K-CLASH) to search for evidence of quenching in massive galaxy clusters at redshifts $0.3

Keywords:

• Astrophysics
• Ram pressure
• Star formation
• Physics
• Galaxy cluster
• Supernova
• Astronomy
• Emission spectrum
• Galaxy
• Interstellar medium
• Redshift

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