most citedGrids of stellar models with rotation IV. Models from 1.7 to 120 Msun at a metallicity Z = 0.0004

101 citations · 177 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph.SR202027 cited

SNAPSHOT: Connections between Internal and Surface Properties of Massive Stars

Eoin Farrell, Jose Groh, Georges Meynet +3

We introduce SNAPSHOT, a technique to systematically compute stellar structure models in hydrostatic and thermal equilibrium based on 3 structural properties - core mass $M_{\rm co…

astro-ph.SR2020

The possible disappearance of a massive star in the low metallicity galaxy PHL 293B

Andrew Allan, Jose Groh, Andrea Mehner +4

We investigate a suspected very massive star in one of the most metal-poor dwarf galaxies, PHL~293B. Excitingly, we find the sudden disappearance of the stellar signatures from our…

astro-ph.SR202049 cited

The Uncertain Masses of Progenitors of Core Collapse Supernovae and Direct Collapse Black Holes

Eoin Farrell, Jose Groh, Georges Meynet +1

We show that it is not possible to determine the final mass of a red supergiant (RSG) at the pre-supernova (SN) stage from its luminosity and effective temperatur…

astro-ph.SR2019

Massive black holes regulated by luminous blue variable mass loss and magnetic fields

Jose H. Groh, Eoin Farrell, Georges Meynet +5

We investigate the effects of mass loss during the main-sequence (MS) and post-MS phases of massive star evolution on black hole (BH) birth masses. We compute solar metallicity Gen…

astro-ph.SR2019101 cited

Grids of stellar models with rotation IV. Models from 1.7 to 120 Msun at a metallicity Z = 0.0004

Jose H. Groh, Sylvia Ekström, Cyril Georgy +8

The effects of rotation on stellar evolution are particularly important at low metallicity, when mass loss by stellar winds diminishes and the surface enrichment due to rotational…