An ALMA study of hub-filament systems – I. On the clump mass concentration within the most massive cores

ABSTRACT The physical processes behind the transfer of mass from parsec-scale clumps to massive star-forming cores remain elusive. We investigate the relation between the clump morphology and the mass fraction that ends up in its most massive core (MMC) as a function of infrared brightness, i.e. a c...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2021-12, Vol.508 (2), p.2964-2978
Hauptverfasser:	Anderson, Michael, Peretto, Nicolas, Ragan, Sarah E, Rigby, Andrew J, Avison, Adam, Duarte-Cabral, Ana, Fuller, Gary A, Shirley, Yancy L, Traficante, Alessio, Williams, Gwenllian M
Format:	Artikel
Sprache:	eng
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