paper

DUVET: sub-kiloparsec resolved star formation driven outflows in a sample of local starbursting disk galaxies

arXiv:2402.17830

Abstract

We measure resolved (kiloparsec-scale) outflow properties in a sample of 10 starburst galaxies from the DUVET (Deep near-UV observations of Entrained gas in Turbulent galaxies) sample, using Keck/KCWI observations of H and [OIII]~5007. We measure lines-of-sight that contain outflows, and use these to study scaling relationships of outflow velocity (), mass-loading factor (; mass outflow rate per SFR) and mass flux (; mass outflow rate per area) with co-located SFR surface density () and stellar mass surface density (). We find strong, positive correlations of and . We also find shallow correlations between and both and . Our resolved observations do not suggest a threshold in outflows with , but rather we find that the local specific SFR () is a better predictor of where outflows are detected. We find that outflows are very common above ~Gyr and rare below this value. We argue that our results are consistent with a picture in which outflows are driven by supernovae, and require more significant injected energy in higher mass surface density environments to overcome local gravity. The correlations we present here provide a statistically robust, direct comparison for simulations and higher redshift results from JWST.

23 pages, 9 figures, plus 5 figures in the Appendix. Supplementary table of results in Ancillary Files. Resubmitted to MNRAS after referee report

DUVET: sub-kiloparsec resolved star formation driven outflows in a sample of local starbursting disk galaxies · wovepaper