The t tauri phase down to nearly planetary masses : Echelle spectra of 82 very low mass stars and brown dwarfs

@article{Mohanty2005TheTT,
  title={The t tauri phase down to nearly planetary masses : Echelle spectra of 82 very low mass stars and brown dwarfs},
  author={S. Mohanty and R. Jayawardhana and G. Basri},
  journal={The Astrophysical Journal},
  year={2005},
  volume={626},
  pages={498-522}
}
Using the largest high-resolution spectroscopic sample to date of young, very low mass stars and brown dwarfs, we investigate disk accretion in objects ranging from just above the hydrogen-burning limit all the way to nearly planetary masses. Our 82 targets span spectral types from M5 to M9.5, or masses from 0.15 M? down to about 15 jupiters. They are confirmed members of the ? Ophiuchus, Taurus, Chamaeleon I, IC 348, R Coronae Australis, Upper Scorpius, and TW Hydrae star-forming regions and… Expand

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