SEDIGISM: Structure, excitation, and dynamics of the inner Galactic interstellar medium
Article 2017 en
Authors
FS
F. Schüller
TC
T. Csengeri
JU
J. S. Urquhart
Abstract
1 min read
Context. The origin and life-cycle of molecular clouds are still poorly constrained, despite their importance for understanding the evolution of the interstellar medium. Many large-scale surveys of the Galactic plane have been conducted recently, allowing for rapid progress in this field. Nevertheless, a sub-arcminute resolution global view of the large-scale distribution of molecular gas, from the diffuse medium to dense clouds and clumps, and of their relationshipto the spiral structure, is still missing.
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