Evolution of stars with 60 and 200 M⊙: predictions for WNh stars in the Milky Way

Evolution models done with the Geneva-evolution-code, for the article «Evolution of stars with 60 and 200 M⊙: predictions for WNh stars in the Milky Way»

Authors

A. C. Gormaz-Matamala (ORCID: https://orcid.org/0000-0002-2588-2391)
Amedeo Romagnolo

Institutions

Czech Academy of Sciences (CZ)
Nicolaus Copernicus Astronomical Center (PL)

Publication Details

Journal: Zenodo (CERN European Organization for Nuclear Research)
Published: 2025-03-03
DOI: https://doi.org/10.5281/zenodo.18174053
Primary Topic: Stellar, planetary, and galactic studies
Type: article
Field-Weighted Citation Impact: 0.00

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article

Evolution of stars with 60 and 200 M⊙: predictions for WNh stars in the Milky Way

A. C. Gormaz-Matamala, Amedeo Romagnolo

Mar 3, 2025

Zenodo (CERN European Organization for Nuclear Research)

Stellar, planetary, and galactic studies

article

Evolution of stars with 60 and 200 M⊙: predictions for WNh stars in the Milky Way

A. C. Gormaz-Matamala, Amedeo Romagnolo

March 3, 2025article en

Abstract

Evolution models done with the Geneva-evolution-code, for the article «Evolution of stars with 60 and 200 M⊙: predictions for WNh stars in the Milky Way»

Zenodo (CERN European Organization for Nuclear Research)

Czech Academy of Sciences (CZ), Nicolaus Copernicus Astronomical Center (PL)

Openalex Percentile: Top 28%

Stellar, planetary, and galactic studies

DOI Open Access PDF OpenAlex

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Evolution of stars with 60 and 200 M⊙: predictions for WNh stars in the Milky Way — A. C. Gormaz-Matamala, Amedeo Romagnolo · Zenodo (CERN European Organization for Nuclear Research) (2025) | TGRS Research Map | TGRS