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- W3207091279 abstract "We present a large-scale study of stellar rotation for T Tauri stars in the Orion Star-Forming Complex. We use the projected rotational velocity ($vsin(i)$) estimations reported by the APOGEE-2 collaboration as well as individual masses and ages derived from the position of the stars in the HR diagram, considering Gaia-EDR3 parallaxes and photometry plus diverse evolutionary models. We find an empirical trend for $vsin(i)$ decreasing with age for low-mass stars ($0.4 M_{odot} < M_{ast} < 1.2 M_{odot}$). Our results support the existence of a mechanism linking $vsin(i)$ to the presence of accreting protoplanetary disks, responsible for regulating stellar rotation in timescales of about 6 Myr, which is the timescale in which most of the T Tauri stars lose their inner disk. Our results provide important constraints to models of rotation in the early phases of evolution of young stars and their disks." @default.
- W3207091279 created "2021-10-25" @default.
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- W3207091279 date "2021-12-01" @default.
- W3207091279 modified "2023-10-17" @default.
- W3207091279 title "Stellar Rotation of T Tauri Stars in the Orion Star-forming Complex" @default.
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