Browsing by Author "Flores, C."

Now showing items 1-3 of 3

    • A highly settled disk around Oph163131 
      Villenave, M.; Stapelfeldt, K. R.; Duchêne, G.; Ménard, F.; Lambrechts, M.; Sierra Morales, Anibal; Flores, C.; Dent, W. R. F.; Wolff, S.; Ribas, A.; Benisty, Myriam; Cuello, N.; Pinte, C. (IOP, 2022)
      High dust density in the midplane of protoplanetary disks is favorable for efficient grain growth and can allow fast formation of planetesimals and planets, before disks dissipate. Vertical settling and dust trapping in ...
    • Planet Formation Signposts: Observability of Circumplanetary Disks via Gas Kinematics 
      Pérez, Sebastián; Dunhill, A.; Casassus Montero, Simón; Roman, P.; Szulágyi, J.; Flores, C.; Marino, S.; Montesino, M. (The American Astronomical Society, 2015-09-20)
      The identification of ongoing planet formation requires the finest angular resolutions and deepest sensitivities in observations inspired by state-of-the-art numerical simulations. Hydrodynamic simulations of planet–dis ...
    • Planet Formation Signposts: Observability of Circumplanetary Disks Via Gas Kinematics 
      Pérez, Sebastián; Dunhill, A.; Casassus Montero, Simón; Román Asenjo, Pablo; Szulágyi, J.; Flores, C.; Marino Estay, Sebastián; Montesinos, Matías (IOP, 2015)
      The identification of on-going planet formation requires the finest angular resolutions and deepest sensitivities in observations inspired by state-of-the-art numerical simulations. Hydrodynamic simulations of ...