Planet formation around intermediate-mass stars. I. Different disc evolutionary pathways as a function of stellar mass
Context. The study of protoplanetary disc evolution and theories of planet formation has predominantly concentrated on solar- (and low-) mass stars since they host the majority of confirmed exoplanets. Nevertheless, the confirmation of numerous planets orbiting stars more massive than the Sun (up to ~3 M ⊙) has sparked considerable interest in
Ronco, M. P. et al.
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2024