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Star formation rates (SFRs) obtained via extinction corrected H alpha arecompared to dense gas as traced by CO(J=3-2) emission at the centers of nearbygalaxies, observed with the ASTE telescope. It is found that, although many ofthe observed positions are dusty and therefore heavily absorbed at H alpha, theSFR shows a striking correlation with dense gas in the form of the Schmidt lawwith an index 1.0. The correlation is also compared between gas traced byCO(J=1-0) and application of H alpha extinction correction. We find that densegas produces a far better correlation with SFR in view of surface densityvalues.Comment: 6 pages, PASJ accepte

ASTE Observations of Nearby Galaxies: A Tight Correlation between CO J = 3–2 Emission and H$\alpha$