The ALMaQUEST Survey. VII. Star Formation Scaling Relations of Green Valley Galaxies

We utilize the ALMA-MaNGA QUEnch and STar formation (ALMaQUEST) survey to investigate kpc-scale scaling relations, presented as resolved star forming main sequence (rSFMS: $\Sigma_{\rm SFR}$ vs. $\Sigma_{*}$), Schmidt-Kennicutt relation (rSK: H_{2}}$), molecular gas (rMGMS: H_{2}}$ for 11478 star-forming 1414 retired spaxels (oversampled by a factor of $\sim20$) located in 22 green valley (GV) 12 (MS) galaxies. For given galaxy type (MS or GV), are found be offset from sequences formed on rSFMS, rSK, rMGMS planes, toward lower absolute values sSFR, SFE, $f_{\rm $\sim$ 1.1, 0.6, 0.5 dex. The relations GV galaxies distinct that MS galaxies, even if analyses restricted only. It is spaxels, reduced $\sim$0.36, 0.14, 0.21 dex, respectively, compared those Therefore, suppressed sSFR/SFE/$f_{\rm associated with not only an increased proportion regions but also depletion these quantities regions. Finally, reduction SFE relative seen both bulge disk (albeit larger uncertainties), suggesting statistically, quenching population may persist inner outer