Spatially Resolving Galaxy Environmental Quenching in the SAMI Galaxy Survey
In order to identify how spatially resolved star formation depends on environment, we use the unitless scale-radius ratio (r50,Hα/r50,cont) (building on earlier work of Schaefer et al. 2017). We will use this metric to investigate quenching across a much enlarged dynamic range of environment (from c...
Main Authors: | , |
---|---|
Format: | Still Image |
Language: | unknown |
Published: |
Zenodo
2019
|
Subjects: | |
Online Access: | https://dx.doi.org/10.5281/zenodo.2635355 https://zenodo.org/record/2635355 |