Accretion and the Evolution of T Tauri Disks

@inproceedings{AOLA1998AccretionAT,
  title={Accretion and the Evolution of T Tauri Disks},
  author={AOLA and Artmann and ALVET and ULLBRING and LESSIO},
  year={1998}
}
  • AOLA, Artmann, +2 authors LESSIO
  • Published 1998
Using results and calibrations from a previous paper (Gullbring et al. 1997), we estimate disk accretion rates for preÈmain-sequence stars in the Taurus and Chamaeleon I molecular cloud complexes. The median accretion rate for T Tauri stars of age D1 Myr is D10~8 yr~1 ; the intrinsic scatter at a M _ given age may be as large as 1 order of magnitude. There is a clear decline of mass accretion rates M0 with increasing age t among T Tauri stars. Representing this decline as we estimate M0 P t~g… CONTINUE READING
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Sequence Objects, ed

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