Line emission from filaments in molecular clouds

ABSTRACT Filamentary structures are often identified in column density maps of molecular clouds, and appear to be important for both low- and high-mass star formation. Theoretically, these structures are expected to form in regions where the supersonic cloud-scale turbulent velocity field converges....

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2023-05, Vol.522 (3), p.3890-3897
Hauptverfasser:	Priestley, F D, Arzoumanian, D, Whitworth, A P
Format:	Artikel
Sprache:	eng
Online-Zugang:	Volltext
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