45 citations · 94 across the 5 of their papers we have counts for
5 papers
A framework for modelling Population III stars in cosmological simulations
Bipradeep Saha, Rahul Kannan, Giovanni M. Mirouh
Population III (Pop III) stars are the first generation of stars to form in the universe, emerging from primordial gas composed mainly of hydrogen and helium. They play a crucial r…
The mass distribution of the first stars can be determined via the 21-cm signal
T. Gessey-Jones, N. S. Sartorio, H. T. J. Bevins +6
The formation of the first stars and the subsequent population of X-ray binaries represents a fundamental transition in the state of the Universe as it evolves from near homogeneit…
Detailed equilibrium and dynamical tides: impact on circularization and synchronization in open clusters
Giovanni M. Mirouh, David D. Hendriks, Sophie Dykes +2
Binary stars evolve into chemically-peculiar objects and are a major driver of the Galactic enrichment of heavy elements. During their evolution they undergo interactions, includin…
Population III X-ray Binaries and their Impact on the Early Universe
Nina S. Sartorio, A. Fialkov, T. Hartwig +8
The first population of X-ray binaries (XRBs) is expected to affect the thermal and ionization states of the gas in the early Universe. Although these X-ray sources are predicted t…
Impact of the Primordial Stellar Initial Mass Function on the 21-cm Signal
T. Gessey-Jones, N. S. Sartorio, A. Fialkov +6
Properties of the first generation of stars (Pop III), such as their initial mass function (IMF), are poorly constrained by observations and have yet to converge between simulation…