Dark-matter halo mergers as a fertile environment for low-mass Population III star formation

TY - JOUR

T1 - Dark-matter halo mergers as a fertile environment for low-mass Population III star formation

AU - Bovino, S.

AU - Latif, M. A.

AU - Grassi, Tommaso

AU - Schleicher, D. R. G.

PY - 2014/6

Y1 - 2014/6

N2 - While Population III (Pop III) stars are typically thought to be massive, pathways towards lower mass Pop III stars may exist when the cooling of the gas is particularly enhanced. A possible route is enhanced HD cooling during the merging of dark-matter haloes. The mergers can lead to a high ionization degree catalysing the formation of HD molecules and may cool the gas down to the cosmic microwave background temperature. In this paper, we investigate the merging of mini-haloes with masses of a few 105Mȯ and explore the feasibility of this scenario. We have performed three-dimensional cosmological hydrodynamics calculations with the ENZO code, solving the thermal and chemical evolution of the gas by employing the astrochemistry package KROME. Our results show that the HD abundance is increased by two orders of magnitude compared to the no-merging case and the halo cools down to ~60K triggering fragmentation. Based on Jeans estimates, the expected stellar masses are about 10Mȯ. Our findings show that the merging scenario is a potential pathway for the formation of low-mass stars.

AB - While Population III (Pop III) stars are typically thought to be massive, pathways towards lower mass Pop III stars may exist when the cooling of the gas is particularly enhanced. A possible route is enhanced HD cooling during the merging of dark-matter haloes. The mergers can lead to a high ionization degree catalysing the formation of HD molecules and may cool the gas down to the cosmic microwave background temperature. In this paper, we investigate the merging of mini-haloes with masses of a few 105Mȯ and explore the feasibility of this scenario. We have performed three-dimensional cosmological hydrodynamics calculations with the ENZO code, solving the thermal and chemical evolution of the gas by employing the astrochemistry package KROME. Our results show that the HD abundance is increased by two orders of magnitude compared to the no-merging case and the halo cools down to ~60K triggering fragmentation. Based on Jeans estimates, the expected stellar masses are about 10Mȯ. Our findings show that the merging scenario is a potential pathway for the formation of low-mass stars.

U2 - 10.1093/mnras/stu714

DO - 10.1093/mnras/stu714

M3 - Journal article

SN - 0035-8711

VL - 441

SP - 2181

EP - 2187

JO - Royal Astronomical Society. Monthly Notices

JF - Royal Astronomical Society. Monthly Notices

IS - 3

ER -