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UV bright red-sequence galaxies: a comparative study between UV upturn and UV weak systems
[article]
2020
arXiv
pre-print
Ultraviolet (UV) emission from galaxies is associated with hot components, whether from stellar sources or not. By making use of colour-colour diagrams, early-type galaxies (ETGs) can be classified in terms of their UV emission in mainly three categories: residual star-formation, UV weak, and UV upturn. This thesis aims at investigating galaxies presenting UV upturn by comparing them to UV weak systems. This investigation has three fronts: (i) the assessment of the evolution in redshift (z) and
arXiv:2011.06476v1
fatcat:lllfsicosvhqpmf6fneakxlysy