Radial distribution of the carbonaceous nano-grains in the protoplanetary disk around HD 169142

@article{Devinat2022RadialDO,
  title={Radial distribution of the carbonaceous nano-grains in the protoplanetary disk around HD 169142},
  author={M. Devinat and 'Emilie Habart and 'Eric Pantin and Nathalie Ysard and Anthony P. Jones and Lucas Labadie and Emmanuel di Folco},
  journal={Astronomy \& Astrophysics},
  year={2022}
}
Context. HD 169142 is part of the class of (pre-)transitional protoplanetary disks showing multiple carbon nanodust spectroscopic signatures (aromatic, aliphatic) dominating the infrared spectrum. Precise constraints on the spatial distribution and properties of carbonaceous dust particles are essential to understanding the physics, radiative transfer processes, and chemistry of the disk. The HD 169142 disk is seen almost face-on and thus it o ff ers a unique opportunity to study the dust radial… 

References

SHOWING 1-2 OF 2 REFERENCES

VizieR Online Data Catalog: I/337

  • 2016