From blue cloud to red sequence: evidence of morphological transition prior to star formation quenching
We present a study of a sample of 254 clusters from the SDSS-DR7 Yang Catalogue and an auxiliary sample of field galaxies to perform a detailed investigation on how galaxy quenching depends on both environment and galaxy stellar mass. Our samples are restricted to 0.03 ≤ z ≤ 0.1 and we only consider clusters with log (M halo/M ⊙) ≥ 14. Comparing
Sampaio, V. M. et al.
Fecha de publicación:
1
2022