We compare 500~pc scale, resolved observations of ionised and molecular gas
for the z∼0.02 starbursting disk galaxy IRAS08339+6517, using measurements
from KCWI and NOEMA. We explore the relationship of the star formation driven
ionised gas outflows with colocated galaxy properties. We find a roughly linear
relationship between the outflow mass flux (Σ˙out) and star
formation rate surface density (ΣSFR), Σ˙out∝ΣSFR1.06±0.10, and a strong correlation between
Σ˙out and the gas depletion time, such that
Σ˙out∝tdep−1.1±0.06. Moreover, we find these
outflows are so-called ``breakout" outflows, according to the relationship
between the gas fraction and disk kinematics. Assuming that ionised outflow
mass scales with total outflow mass, our observations suggest that the regions
of highest ΣSFR in IRAS08 are removing more gas via the outflow
than through the conversion of gas into stars. Our results are consistent with
a picture in which the outflow limits the ability for a region of a disk to
maintain short depletion times. Our results underline the need for resolved
observations of outflows in more galaxies.Comment: 16 pages, 7 figures, Submitted to Ap