Skip to main content
SearchLogin or Signup

Closing Gaps in Our Astrochemical Heritage: From Molecular Clouds to Planets

Published onMay 31, 2019
Closing Gaps in Our Astrochemical Heritage: From Molecular Clouds to Planets
·

Abstract

We discuss the observational needs in the coming decade to enable the robust interpretation of chemical evolution from molecular clouds through to the formation of planets, especially in sources such as protoplanetary disks and exoplanet atmospheres, where only the simplest of species can be directly observed.

The full text of this article is only available in PDF format:



Comments
0
comment

No comments here