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20182022
most citedEvolution of Wolf-Rayet stars as black hole progenitors

44 citations · 77 across the 3 of their papers we have counts for

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Showing astro-ph.SRShow all

6 papers · 1 filter

astro-ph.SR20227 cited

Stellar age determination in the Mass-Luminosity Plane

Erin R. Higgins, Jorick S. Vink

The ages of stars have historically relied on isochrone fitting of standardised grids of models. While these stellar models have provided key constraints on observational samples o…

astro-ph.SR202126 cited

Superadiabaticity and the metallicity independence of the Humphreys-Davidson limit

Gautham N. Sabhahit, Jorick S. Vink, Erin R. Higgins +1

The Humphreys-Davidson (HD) limit sets the boundary between evolutionary channels of massive stars that either end their lives as red supergiants (RSGs) or as the hotter blue super…

astro-ph.SR202144 cited

Evolution of Wolf-Rayet stars as black hole progenitors

Erin R. Higgins, Andreas A. C. Sander, Jorick S. Vink +1

Evolved Wolf-Rayet stars form a key aspect of massive star evolution, and their strong outflows determine their final fates. In this study, we calculate grids of stellar models for…

astro-ph.SR2020

A theoretical investigation of the Humphreys-Davidson limit at high and low metallicity

Erin R. Higgins, Jorick S. Vink

Current massive star evolution grids are not able to simultaneously reproduce the empirical upper luminosity limit of red supergiants, the Humphrey-Davidson (HD) limit at high and…

astro-ph.SR2018

Massive star evolution : rotation, winds, and overshooting vectors in the Mass-Luminosity plane I. A calibrated grid of rotating single star models

Erin R. Higgins, Jorick S. Vink

We aim to constrain massive star evolution models using the unique testbed eclipsing binary HD166734 with new grids of MESA stellar evolution models, adopting calibrated prescripti…

astro-ph.SR2018

Massive star evolution revealed in the Mass-Luminosity plane

Erin R. Higgins, Jorick S. Vink

Massive star evolution is dominated by key physical processes such as mass loss, convection and rotation, yet these effects are poorly constrained, even on the main sequence. We ut…