H II regions and high-mass starless clump candidates

Context. The ionization feedback from H II regions modifies the properties of high-mass starless clumps (HMSCs, of several hundred to a few thousand solar masses with a typical size of 0.1–1 pc), such as dust temperature and turbulence, on the clump scale. The question of whether the presence of H I...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2021-02, Vol.646
Hauptverfasser:	Zhang, S, Zavagno, A, López-Sepulcre, A, Liu, H, Louvet, F, Figueira, M, Russeil, D, Y. Wu, Yuan, J, Pillai, T G S
Format:	Artikel
Sprache:	eng
Schlagworte:	Angular resolution Clumps Dust Fragmentation H II regions Morphology Spatial distribution Star & galaxy formation Star formation Turbulence
Online-Zugang:	Volltext
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