1. Millimeter interferometric investigations of the energy sources of nearby ULIRGs Masa Imanishi （ NAO Japan ）

2. NLR Buried AGNs ULIRGs: powerful energy sources hidden behind dust Obscured by torus-shaped dust

3. Buried AGNs (=X-ray source) produce XDRs HCN/HCO+ HCN/CO starburst pure AGN XDRs and PDRs(starbursts) are distinguishable from mm line ratios

4. ULIRGs with buried AGNs ULIRGs without buried AGNs Pure AGN Starburst

5. The AGN-nuclear starburst connections in Seyfert 1 and 2 galaxies Masa Imanishi （ NAO Japan ）

6. Nuclear stabursts in a dusty torus Dust torus is rich in molecular gas Nuclear starbursts may occur Sy1 Sy2 PAH 3.3um PAH 3.3um PAH PAH = starburst tracer

7. L(3.3 PAH) = nuclear starburst Nuclear N-band, radio core = AGN power nuclear starburst luminosity : Sy1s = Sy2s L(nuclear starburst) and L(AGN): correlate Imanishi 2003 ApJ 599 918 Imanishi and Wada 2004 ApJ 617 214