Water: from clouds to planets

@article{Dishoeck2014WaterFC,
  title={Water: from clouds to planets},
  author={E. Dishoeck and E. Bergin and D. Lis and J. Lunine},
  journal={arXiv: Astrophysics of Galaxies},
  year={2014},
  pages={835-858}
}
Results from recent space missions, in particular Spitzer and Herschel, have led to significant progress in our understanding of the formation and transport of water from clouds to disks, planetesimals, and planets. [n this review, we provide the underpinnings for the basic molecular physics and chemistry of water and outline these advances in the context of water formation in space, its transport to a forming disk, its evolution in the disk, and finally the delivery to forming terrestrial… Expand
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References

SHOWING 1-8 OF 8 REFERENCES
Extrasolar Carbon Planets
Protostars and Planets IV, p. 1019
  • Kuchner M. J. (2003) Astrophys. J. Lett.,
  • 2000
Protostars and Planets III, (edited by E
  • 2013
2012)Earth and Planetary Science Letters
  • 2012
2004)Atmospheric chemistry and physics
  • 2004
Annual Review of Earth and Planetary Sciences
Earth and Planetary Science Letters
  • Lingling Ye, Hiroo Kanamori, Jean-Philippe Avouac, Linyan Li, Kwok Fai Cheung, Thorne Lay