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    SPIN EVOLUTION OF CLASSICAL T TAURI STARS
    Chinese Science Bulletin (1996)
    Xiang‐Dong LiZhenru Wang
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    Abstract:
    Classical T Tauri stars (hereinafter CTTS) are protostars formed by collapse of molecular clouds. As they evolve towards the main sequence, CCTS accrete from the circumstellar matter and contract due to self-gravitation. Mass accretion and gravitational contraction can accelerate the spin velocities of CTTS up to break-up (～300—400km·s) within
    Keywords:
    Protostar
    Accretion disc
    Circumstellar disk
    Topics:
    Astro and Planetary Science
    Astrophysics and Star Formation Studies
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