ALMA chemical survey of disk-outflow sources in Taurus (ALMA-DOT)

@article{Podio2020ALMACS,
  title={ALMA chemical survey of disk-outflow sources in Taurus (ALMA-DOT)},
  author={Linda Podio and Antonio Garufi and Claudio Codella and Davide Fedele and Eugenio Bianchi and Francesca Bacciotti and Cecilia Ceccarelli and C{\'e}cile Favre and Seyma Mercimek and Kazi L. J. Rygl and Leonardo Testi},
  journal={Astronomy and Astrophysics},
  year={2020},
  volume={642}
}
The chemical composition of planets is inherited from that of the protoplanetary disk at the time of planet formation. Increasing observational evidence suggests that planet formation occurs in less than 1 Myr. This motivates the need for spatially resolved spectral observations of Class I disks, as carried out by the ALMA chemical survey of Disk-Outflow sources in Taurus (ALMA-DOT). In the context of ALMA-DOT, we observe the edge-on disk around the Class I source IRAS 04302+2247 (the butterfly… 

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