Stability of dusty rings in protoplanetary discs

Dust rings in protoplanetary discs are often observed in thermal dust emission and could be fa v ourable environments for planet formation. While dust rings readily form in gas pressure maxima, their long-term stability is key to both their observability and potential to assist in planet formation. We investigate the stability of the dust...

Large-amplitude motion responses of a Ro-Ro ship to regular oblique waves in intact and damaged conditions

Investigation of motions of catamarans in regular waves-II

Investigation of motions of catamarans in regular waves-I

Two-dimensional calculations of the motion of floating bodies

Explosions due to pressurized spheres at the ocean surface

Explosions due to pressurized spheres at the ocean surface