Accretion of pristine gas and dilution during the formation of multiple-population globular clusters

We study the interaction of the early spherical GC wind powered by Type II supernovae (SNe II) with the surrounding ambient medium consisting of the gaseous disc of a star-forming galaxy at redshift z ≳ 2. The bubble formed by the wind eventually breaks out of the disc, and most of the wind moves di...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2016-10, Vol.461 (4), p.4088-4098
Hauptverfasser:	D'Ercole, A., D'Antona, F., Vesperini, E.
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Astronomy Asymptotic properties Clusters Disks Ejecta Formations Galaxies Gases Iron Star & galaxy formation Stars Supernovae Wind
Online-Zugang:	Volltext
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