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...
Autors principals: | Vaughan, SP, Tiley, AL, Davies, RL, Prichard, LJ, Croom, SM, Bureau, M, Stott, JP, Bunker, A, Cappellari, M, Ansarinejad, B, Jarvis, MJ |
---|---|
Format: | Journal article |
Idioma: | English |
Publicat: |
Oxford University Press
2020
|
Ítems similars
-
K-CLASH: spatially-resolving star-forming galaxies in field and cluster environments at z ≈ 0.2-0.6
per: Tiley, AL, et al.
Publicat: (2020) -
CO Tully–Fisher relation of star-forming galaxies at = 0.05–0.3
per: Topal, S, et al.
Publicat: (2018) -
The evolution of gas-phase metallicity and resolved abundances in star-forming galaxies at z ≈ 0.6 – 1.8
per: Gillman, S, et al.
Publicat: (2020) -
Alternating current magnetotransport in Sm0.1La0.6Sr0.3MnO3
per: M. Aparnadevi, et al.
Publicat: (2013-01-01) -
Dielectric properties of La0.67sr0.33Mnl-xTix03 with x = 0.4 and 0.6.
per: Zalita , Z., et al.
Publicat: (2011)