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 Kazi L. J. Rygl and C{\'e}cile Favre and Francesca Bacciotti and Eleonora Bianchi and Cecilia Ceccarelli and Seyma Mercimek and Richard Teague and Leonardo Testi},
  journal={Astronomy \& Astrophysics},
  year={2020}
}
Context.Planets form in protoplanetary disks and inherit their chemical composition. It is therefore crucial to understand the molecular content of protoplanetary disks in their gaseous and solid components.Aims.We aim to characterize the distribution and abundance of molecules in the protoplanetary disk of DG Tau and to compare them with its dust distribution.Methods.In the context of the ALMA chemical survey of Disk-Outflow sources in the Taurus star forming region (ALMA-DOT) we analyze ALMA… Expand

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References

SHOWING 1-10 OF 84 REFERENCES
ALMA chemical survey of disk-outflow sources in Taurus (ALMA-DOT)
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 lessExpand
2020b, arXiv e-prints
  • A&A,
  • 2021
The 2014 ALMA Long Baseline Campaign: First Results from High Angular Resolution Observations toward the HL TAU Region
We present Atacama Large Millimeter/submillimeter Array (ALMA) observations from the 2014 Long Baseline Campaign in dust continuum and spectral line emission from the HL Tau region. The continuumExpand
ALMA chemical survey of disk-outflow sources in Taurus (ALMA-DOT)
Aims: To trace the radial and vertical spatial distribution of H2CS, a key species of the S-bearing chemistry, in protoplanetary disks. To analyse the observed distributions in light of the H2CSExpand
ALMA chemical survey of disk-outflow sources in Taurus (ALMA-DOT)
The chemical composition of planets is inherited by the distribution of the various molecular species in the protoplanetary disk at thetime of their formation. As of today, only a handful of disksExpand
ALMA reveals a large structured disk and nested rotating outflows in DG Tauri B
We present Atacama Large Millimeter Array (ALMA) Band 6 observations at 14-20 au spatial resolution of the disk and CO(2-1) outflow around the Class I protostar DG Tau B in Taurus. The disk is veryExpand
An ALMA Survey of H2CO in Protoplanetary Disks
H₂CO is one of the most abundant organic molecules in protoplanetary disks and can serve as a precursor to more complex organic chemistry. We present an Atacama Large Millimeter/submillimeter ArrayExpand
An Unbiased ALMA Spectral Survey of the LkCa 15 and MWC 480 Protoplanetary Disks
The volatile contents of protoplanetary disks both set the potential for planetary chemistry and provide valuable probes of defining disk system characteristics such as stellar mass, gas mass,Expand
Binding Energies of Interstellar Molecules on Crystalline and Amorphous Models of Water Ice by Ab Initio Calculations
In the denser and colder ($\leq$20 K) regions of the interstellar medium (ISM), near-infrared observations have revealed the presence of sub-micron sized dust grains covered by several layers ofExpand
Measuring elemental abundance ratios in protoplanetary disks at millimeter wavelengths
Over million years of evolution, gas dust and ice in protoplanetary disks can be chemically reprocessed. There is evidence that the gas-phase carbon and oxygen abundances are subsolar in disksExpand
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