Genesis and evolution of dust in galaxies in the early Universe - I. Modelling dust evolution in starburst galaxies

Free Access

Table 4

EIT08M exceeding 10⁸M_⊙ of dust within ~400–500 Myr.

M_ini	ϵ_SN	M_cl	IMF

1.3 × 10¹²M_⊙	max	0	all
	max	100	all
	max	800	all
	high	0	all
	high	100	all
	low	0	mass-heavy, Larson 1
	low	100	mass-heavy, Larson 1
5 × 10¹¹M_⊙	max	0	all
	max	100	all
	max	800	all
	high	0	all
	high	100	top-heavy, Larson 1, 2, mass-heavy
	low	0	mass-heavy
1 × 10¹¹M_⊙	max	0	all
	max	100	top-heavy, Larson 1, 2, mass-heavy
	high	0	Larson 2
5 × 10¹⁰M_⊙	max	0	top-heavy, Larson 1, 2, mass-heavy
	max	100	Larson 2
	max^a	100	top-heavy, Larson 1, mass-heavy

Notes.

^(a)

Top-heavy IMF: only within the first ~300 Myr, Larson 1 and mass-heavy IMF only within the first ~100 Myr.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.