activity
20222026
most citedGrids of stellar models with rotation VI: Models from 0.8 to 120 at a metallicity Z = 0.006

68 citations · 185 across the 31 of their papers we have counts for

collaborators
Showing 2024Show all

7 papers · 1 filter

astro-ph.GA2024★ 2 cited

The Origin of Supermassive Black Holes from Pop III.1 Seeds

Jonathan C. Tan, Jasbir Singh, Vieri Cammelli +4

The origin of supermassive black holes (SMBHs) is a key open question for contemporary astrophysics and cosmology. Here we review the features of a cosmological model of SMBH forma…

astro-ph.SR2024★ 1 cited

Grids of stellar models with rotation VIII: Models from 1.7 to 500 at metallicity

Yves Sibony, Kendall G. Shepherd, Norhasliza Yusof +12

Grids of stellar evolution models with rotation using the Geneva stellar evolution code (Genec) have been published for a wide range of metallicities. We introduce the last remaini…

astro-ph.SR2024★ 12 cited

The Evolution of Accreting Population III Stars at 10-10 M/yr

Devesh Nandal, Lorenz Zwick, Daniel J. Whalen +3

The first stars formed over five orders of magnitude in mass by accretion in primordial dark matter halos. We study the evolution of massive, very massive and supermassive primordi…

astro-ph.HE2024★ 7 cited

Linear adiabatic analysis for general relativistic instability in primordial accreting supermassive stars

Hideyuki Saio, Devesh Nandal, Sylvia Ekstroem +1

Accreting supermassive stars of will eventually collapse directly to a black hole via the general relativistic (GR) instability. Such direct collapses of…

astro-ph.GA2024★ 29 cited

Fast-rotating massive Population~III stars as possible sources of extreme N-enrichment in high-redshift galaxies

Devesh Nandal, Yves Sibony, Sophie Tsiatsiou

We present an analysis of the chemical compositions in high-redshift galaxies, with a focus on the nitrogen-enhanced galaxies GN-z11 and CEERS-1019. We use stellar models of massiv…

astro-ph.SR2024★ 24 cited

Rapidly rotating Population III stellar models as a source of primary nitrogen

Sophie Tsiatsiou, Yves Sibony, Devesh Nandal +12

The first stars might have been fast rotators. This would have important consequences for their radiative, mechanical and chemical feedback. We discuss the impact of fast initial r…

astro-ph.GA2024★ 1 cited

Explaining the high nitrogen abundances observed in high-z galaxies via population III stars of a few thousand solar masses

Devesh Nandal, John A. Regan, Tyrone E. Woods +3

The chemical enrichment of the early Universe is a crucial element in the formation and evolution of galaxies, and Population III (PopIII) stars must play a vital role in this proc…