We examine the relation between star formation and dense gas, traced by HCN (1–0), using a sample of 343 Galactic clumps spanning the full range of evolutionary stages representative of high-mass and cluster formation, including quiescent, protostellar, young stellar object (YSO), and H ii regions. Earlier Galactic s...
I. Grozdanova, J. Urquhart, W.-J. Kim et al.· Monthly notices of the Royal...· 0 citations
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