Radiative Transfer SPH Simulations of UV Feedback on Pop III Star Formation

Details Radiative Transfer SPH Simulations of UV Feedback on Pop III Star Formation Radiative Transfer SPH Simulations of UV Feedback on Pop III Star Formation

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc..990..393s&link_type=abstract

FIRST STARS III: First Stars II Conference. AIP Conference Proceedings, Volume 990, pp. 393-394 (2008).

Mathematics

Logic

Population Iii Stars, Star Formation, Hii Regions, Emission And Reflection Nebulae, Hydrodynamics, Numerical Simulation, Solution Of Equations

Scientific paper

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 Msolar 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.

Affiliated with

Also associated with

No associations

Rating

Radiative Transfer SPH Simulations of UV Feedback on Pop III Star Formation does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Radiative Transfer SPH Simulations of UV Feedback on Pop III Star Formation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radiative Transfer SPH Simulations of UV Feedback on Pop III Star Formation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1037024