The chemical structure of young high-mass star-forming clumps: (I) Deuteration

31 Aug 2019 Feng S. Caselli P. Wang K. Lin Y. Beuther H. Sipilä O.

The chemical structure of high-mass star nurseries is important for a general understanding of star formation. Deuteration is a key chemical process in the earliest stages of star formation because its efficiency is sensitive to the environment... (read more)

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  • ASTROPHYSICS OF GALAXIES
  • SOLAR AND STELLAR ASTROPHYSICS