Accretion, disks, and magnetic activity in the TW Hya association

(2) INAF / Osservatorio Astrofisico di Catania; (3) INAF / Osservatorio Astronomico di Capodimonte); A. Frasca (2); B.Stelzer (1); J.M. Alcala (3) ((1) INAF / Osservatorio Astronomico di Palermo

arxiv: 1509.00170 · v1 · pith:3O5RMHIAnew · submitted 2015-09-01 · 🌌 astro-ph.SR

Accretion, disks, and magnetic activity in the TW Hya association

B.Stelzer (1) , A. Frasca (2) , J.M. Alcala (3) ((1) INAF / Osservatorio Astronomico di Palermo , (2) INAF / Osservatorio Astrofisico di Catania , (3) INAF / Osservatorio Astronomico di Capodimonte) This is my paper

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keywords accretionactivityassociationdisksmagneticcircumstellarcomprehensivecritical

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We present new photometric and spectroscopic data for the M-type members of the TW Hya association with the aim of a comprehensive study of accretion, disks and magnetic activity at the critical age of ~10 Myr where circumstellar matter disappears.

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Accretion, disks, and magnetic activity in the TW Hya association

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