activity
20232025
most citedEvolution of rotating massive stars with new hydrodynamic wind models

13 citations · 25 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2025

Revisiting the Evolutionary Status of Massive Stars at the central parsec of the Milky Way

A. C. Gormaz-Matamala, J. Cuadra, B. Kubátová +2

Massive stars and their winds have a large influence in their environment, e.g, determining the accretion rate on to the Galactic Centre (GC) super-massive black hole Sgr A*. The w…

astro-ph.EP2024

Combining REBOUND and MESA: Dynamical Evolution of Planets Orbiting Interacting Binaries

Zepei Xing, Santiago Torres, Ylva Götberg +3

Although planets have been found orbiting binary systems, whether they can survive binary interactions is debated. While the tightest-orbit binaries should host the most dynamicall…

astro-ph.SR2024

Unveiling the structural content of NGC 6357 via kinematics and NIR variability

C. Ordenes-Huanca, M. Zoccali, A. Bayo +3

NGC 6357, a star-forming complex at kpc from the Sun, contains giant molecular clouds and three prominent star clusters alongside with HII regions, very massive stars an…

astro-ph.SR2024★ 12 cited

Evolution of rotating massive stars adopting a newer, self-consistent wind prescription at SMC metallicity

Alex Camilo Gormaz-Matamala, Jorge Cuadra, Sylvia Ekström +3

We use Geneva-evolution-code to run evolutionary tracks for stellar masses ranging from to at SMC metallicity (). We upgrade the recipe for stellar win…

astro-ph.SR2023★ 13 cited

Evolution of rotating massive stars with new hydrodynamic wind models

Alex Camilo Gormaz-Matamala, Jorge Cuadra, Georges Meynet +1

Mass loss due to line-driven winds is central to our understanding of the evolution of massive stars. We extend the evolution models introduced in Paper I, where the mass loss reci…