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- W1622639746 abstract "To explore the radiative feedback from first stars on the subsequent Pop III star formation in a Lambda‐CDM universe, we perform high‐resolution cosmological SPH simulations coupled with radiative transfer of UV radiation, using FIRST simulator. In the simulations, the baryon mass resolution is 0.3 M⊙ and the number of particles is several 105 respectively for baryon and dark matter component. We assume that several collapsing cores form in a Pop III object and one of them evolves into a first star, and then investigate the evolution of other collapsing cores with paying special attention to the radiation hydrodynamic feedback. As a result, it is shown that other collapsing cores are impervious to the negative radiative feedbacks of H2 photodissociation and photoevapolation, but can continue to collapse due to the shielding of UV radiation, consistent with the results of Susa & Umemura (2006). This result implies that all collapsing cores in a Pop III object can evolve into stars." @default.
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- W1622639746 date "2008-01-01" @default.
- W1622639746 modified "2023-09-23" @default.
- W1622639746 title "Radiative Transfer SPH Simulations of UV Feedback on Pop III Star Formation" @default.
- W1622639746 doi "https://doi.org/10.1063/1.2905589" @default.
- W1622639746 hasPublicationYear "2008" @default.
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