2022
DOI: 10.1093/mnras/stac3481
|View full text |Cite
|
Sign up to set email alerts
|

The statistical properties of stars at redshift, z = 5, compared with the present epoch

Abstract: We report the statistical properties of stars and brown dwarfs obtained from three radiation hydrodynamical simulations of star cluster formation with metallicities of 1, 1/10 and 1/100 of the solar value. The star-forming clouds are subjected to cosmic microwave background radiation that is appropriate for star formation at a redshift z = 5. The results from the three calculations are compared to each other, and to similar previously published calculations that had levels of background radiation appropriate f… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1

Citation Types

0
1
0

Year Published

2023
2023
2024
2024

Publication Types

Select...
6

Relationship

0
6

Authors

Journals

citations
Cited by 10 publications
(1 citation statement)
references
References 152 publications
0
1
0
Order By: Relevance
“…A positive correlation between the IMF slope and metallicity is suggested from analytical and numerical simulations (e.g., Omukai et al 2005;Dopcke et al 2013;Chon et al 2021;Guszejnov et al 2022;Bate 2023). Additionally, a nonlinear variation in the IMF with metallicity is proposed owing to the formation of molecules and dust at different metallicities (Chon & Omukai 2020;Sharda & Krumholz 2022).…”
Section: The Metallicity-dependent Imf Hypothesismentioning
confidence: 93%
“…A positive correlation between the IMF slope and metallicity is suggested from analytical and numerical simulations (e.g., Omukai et al 2005;Dopcke et al 2013;Chon et al 2021;Guszejnov et al 2022;Bate 2023). Additionally, a nonlinear variation in the IMF with metallicity is proposed owing to the formation of molecules and dust at different metallicities (Chon & Omukai 2020;Sharda & Krumholz 2022).…”
Section: The Metallicity-dependent Imf Hypothesismentioning
confidence: 93%