Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Andama, Geoffrey"'
Publikováno v:
A&A 683, A118 (2024)
The exoplanet diversity has been linked to the disc environment in which they form, where the host star metallicity and the formation pathways play a crucial role. In the context of the core accretion paradigm, the initial stages of planet formation
Externí odkaz:
http://arxiv.org/abs/2401.16155
Protoplanetary discs exhibit a diversity of gaps and rings of dust material, believed to be a manifestation of pressure maxima commonly associated with an ongoing planet formation and several other physical processes. Hydrodynamic disc simulations fu
Externí odkaz:
http://arxiv.org/abs/2203.09266
Depending on the stellar densities, protoplanetary discs in stellar clusters undergo background heating, disc truncation-driven by stellar encounter, and photo-evaporation. Disc truncation leads to reduced characteristic sizes and disc masses that ev
Externí odkaz:
http://arxiv.org/abs/2202.11935
In the general classical picture of pebble-based core growth, planetary cores grow by accretion of single pebble species. The growing planet may reach the so-called pebble isolation mass, at which it induces a pressure bump that blocks inward driftin
Externí odkaz:
http://arxiv.org/abs/2111.15218