Population III star formation in the presence of turbulence, magnetic fields, and ionizing radiation feedback

Author(s):
Sharda, P. (0000-0003-3347-7094); Menon, S.H.
Published
2025
Publication type
Article / Letter to editor
MHDradiation: dynamicsRadiation mechanisms: generalTurbulenceStars: formationStars: Population III.
Date issued
2025
Language
English
Is part of
Monthly Notices of the Royal Astronomical Society (2025), Vol. 540, no. 2, p. 1745-1764
hdl
1887/4291770
doi
10.1093/mnras/staf803
URL
https://ui.adsabs.harvard.edu/abs/2025MNRAS.540.1745S