Kavli Institute For Astronomy And Astrophysics 1
1. Evolution of star clusters with initial bulk rotation via N -body simulations
2. Evidence for Core-Core Collision in Barnard 68
3. MAJORS II: HCO+and HCN abundances in W40
4. The DRAGON-II simulations – I. Evolution of single and binary compact objects in star clusters with up to 1 million stars
5. The DRAGON-II simulations – III. Compact binary mergers in clusters with up to 1 million stars: mass, spin, eccentricity, merger rate, and pair instability supernovae rate
6. Intermediate-mass ratio inspirals in merging elliptical galaxies
7. On the Scarcity of Dense Cores (n > 105cm-3) in High-latitude Planck Galactic Cold Clumps
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