Condition for dust evacuation from the first galaxies

Hajime Fukushima, Hidenobu Yajima, Kazuyuki Omukai

Research output: Contribution to journalArticlepeer-review

4 Citations (Scopus)

Abstract

Dust enables low-mass stars to form from low-metallicity gas by inducing fragmentation of clouds via cooling by thermal emission. Dust may, however, be evacuated from star-forming clouds due to the radiation force from massive stars. We study here the condition for dust evacuation by comparing the dust evacuation time with the time of cloud destruction due to either expansion of HII regions or supernovae. The cloud destruction time has a weak dependence on cloud radius, while the dust evacuation time is shorter for a cloud with a smaller radius. Dust evacuation, thus, occurs in compact star-forming clouds whose column density is NH ≃ 1024-1026 cm-2. The critical halo mass above which dust evacuation occurs is lower for higher formation red shift, e.g. ~109M at red shift z ~ 3 and ~107M at z ~ 9. In addition, the metallicity of the gas should be less than ~10-2 Z, otherwise attenuation by dust reduces the radiation force significantly. From the dust-evacuated gas, massive stars are likely to form, even with a metallicity above ~10-5 Z, the critical value for low-mass star formation due to dust cooling. This can explain the dearth of ultra-metal-poor stars with a metallicity lower than ~10-4 Z.

Original languageEnglish
Pages (from-to)1071-1085
Number of pages15
JournalMonthly Notices of the Royal Astronomical Society
Volume477
Issue number1
DOIs
Publication statusPublished - 2018 Jun 11

Keywords

  • Dust
  • Extinction
  • Galaxies: Evolution
  • Stars: Formation
  • Stars: Low-mass
  • Stars: Population II

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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