Secular Evolution Via Bar-Driven Gas Inflow: Results from BIMA SONG

We present an analysis of the molecular gas distributions in the 29 barred and 15 unbarred spirals in the BIMA CO (J=1–0) Survey of Nearby Galaxies (SONG). For galaxies that are bright in CO, we confirm the conclusion by Sakamoto et al. (1999b) that barred spirals have higher molecular gas concentrations in the central kiloparsec. The SONG sample also includes 27 galaxies below the CO brightness limit used by Sakamoto et al. Even in these less CO-bright galaxies we show that high central gas concentrations are more common in barred galaxies, consistent with radial inflow driven by the bar. However, there is a significant population of early-type (Sa–Sbc) barred spirals (6 of 19) that have no molecular gas detected in the nuclear region, and have very little out to the bar co-rotation radius. This suggests that in barred galaxies with gas-deficient nuclear regions the bar has already driven most of the gas within the bar co-rotation radius to the nuclear region, where it has been consumed by star formation. The median mass of nuclear molecular gas is over four times higher in early type bars than in late type (Sc–Sdm) bars. Since previous work has shown that the gas consumption rate is an order of magnitude higher in early type bars, this implies that the early types have significantly higher bar-driven inflows. The lower accretion rates in late type bars can probably be attributed to the known differences in Spitzer Science Center, MS 220-6, California Institute of Technology, Pasadena, CA 91125 Department of Astronomy, University of Maryland, College Park, MD 20742-2421 Visiting Astronomer, Kitt Peak National Observatory. KPNO is operated by AURA, Inc. under contract to the National Science Foundation. Email: [email protected] Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 Department of Physics, Bucknell University, Lewisburg, PA 17837