Rotational evolution of solar-type protostars during the star-disk interaction phase

18 Oct 2019 Gallet Florian Zanni Claudio Amard Louis

The early pre-main sequence phase during which they are still likely surrounded by an accretion disk represents a puzzling stage of the rotational evolution of solar-mass stars. While they are still accreting and contracting they do not seem to spin-up substantially... (read more)

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  • SOLAR AND STELLAR ASTROPHYSICS