Reading between the lines

@article{SiciliaAguilar2020ReadingBT,
  title={Reading between the lines},
  author={A. Sicilia-Aguilar and J'erome Bouvier and C. Dougados and Konstantin N. Grankin and Jean-François Donati},
  journal={arXiv: Solar and Stellar Astrophysics},
  year={2020}
}
(Abridged) We use optical spectroscopy to investigate the disk, wind, and accretion during the 2008 ZCMa NW outburst. Over 1000 optical emission lines reveal accretion, a variable, multi-component wind, and double-peaked lines of disk origin. The variable, non-axisymmetric, accretion-powered wind has slow ($\sim $0 km s$^{-1}$), intermediate ($\sim -$100 km s$^{-1}$) and fast ($\geq -$400 km s$^{-1}$) components. The fast components are of stellar origin and disappear in quiescence, while the… Expand
1 Citations
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