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...
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| Format: | Still Image |
| Language: | unknown |
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Zenodo
2019
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| Online Access: | https://dx.doi.org/10.5281/zenodo.2635354 https://zenodo.org/record/2635354 |