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Wladimir Lyra

California Institute of Technology
California State University, Northridge
American Museum of Natural History

161

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5921

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Numerical models of the observability of supernovae in agn disks

2021
- Harrison E. Cook
- Wladimir Lyra
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Can streaming instability followed by pebble accretion explain the density distribution of Kuiper belt objects

2021
- Manuel Cañas
- Wladimir Lyra
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The Initial Conditions for Planet Formation: Turbulence Driven by Hydrodynamical Instabilities in Disks around Young Stars

2021
- Wladimir Lyra
- Orkan Umurhan
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Evolution of MU69 from a binary planetesimal into contact by Kozai-Lidov oscillations and nebular drag

2021
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Assembling Planetary Systems in Starlight-Heated Disks of Gas and Dust

2021
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Vortex Dynamics at the Jovian Pole

2021
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Pebble Trapping in Vortices: Three-dimensional Simulations

2021 The Astrophysical Journal
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Orbital Migration of Interacting Stellar Mass Black Holes in Disks around Supermassive Black Holes II. Spins and Incoming Objects

2020 The Astrophysical Journal
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Evolution of MU69 from a binary planetesimal into contact by Kozai-Lidov oscillations and nebular drag

2020 Icarus
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Evolution of MU69 from a binary planetesimal into contact by Kozai-Lidov oscillations and nebular drag

2020 arXiv: Earth and Planetary Astrophysics
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