Figure 4
Histograms of the ratio of SSFR evaluated within the SDSS fibre to SSFR for the galaxy as a whole (log C(SF)) are shown for the barred galaxy sample (open histograms), and for the control sample matched in stellar mass, stellar mass surface density and g−i colour (red hatched histograms). The plots on the left show results for galaxies with weak bars (ebar < 0.5), while the plots on the right are for galaxies with strong bars (ebar > 0.5). The samples are further divided by stellar mass (log M*, M* is in units of M⊙), stellar mass surface density (log μ*, μ* is in units of M⊙ kpc−2), concentration (R90/R50), g−i colour, asymmetry index (A) and relative bar size (Dbar/Ddisc) at the median value of each parameter as denoted in each plot. Only bar sample A galaxies are plotted.

Histograms of the ratio of SSFR evaluated within the SDSS fibre to SSFR for the galaxy as a whole (log C(SF)) are shown for the barred galaxy sample (open histograms), and for the control sample matched in stellar mass, stellar mass surface density and gi colour (red hatched histograms). The plots on the left show results for galaxies with weak bars (ebar < 0.5), while the plots on the right are for galaxies with strong bars (ebar > 0.5). The samples are further divided by stellar mass (log M*, M* is in units of M), stellar mass surface density (log μ*, μ* is in units of M kpc−2), concentration (R90/R50), gi colour, asymmetry index (A) and relative bar size (Dbar/Ddisc) at the median value of each parameter as denoted in each plot. Only bar sample A galaxies are plotted.

Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close