(56) Production(s) of MARTINS F.

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Massive stars in the Small Magellanic Cloud : Evolution, rotation and surface abundances ![]() Author(s): Bouret Jean-claude, Martins F., Hillier Desmond john, Marcolino Wagner, Rocha-pinto Helio, Georgy Cyril, Lanz Thierry, Hubeny Ivan
(Article) Published:
Astronomy & Astrophysics, vol. 647 p.134 (2021)
Links openAccess full text : |

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The effects of surface fossil magnetic fields on massive star evolution: III. The case of $\tau$ Sco ![]() Author(s): Keszthelyi Z., Meynet G., Martins F., De koter A., David-uraz A.
(Article) Published:
Monthly Notices Of The Royal Astronomical Society, vol. 504 p.2474-2492 (2021)
Links openAccess full text : |

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On the maximum helium content of multiple populations in the globular cluster NGC6752 ![]() Author(s): Martins F., Chantereau William, Charbonnel Corinne
(Document without bibliographic reference) 2021-04-28Links openAccess full text : |

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Spectroscopic evolution of massive stars near the main sequence at low metallicity ![]() Author(s): Martins F., Palacios A.
(Article) Published:
Astronomy & Astrophysics, vol. 645 p.67 (2021)
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Impact of a companion and of chromospheric emission on the shape of chromosome maps for globular clusters ![]() Author(s): Martins F., Morin J., Charbonnel C., Lardo C., Chantereau W. (Article) Published: Astronomy & Astrophysics, vol. 635 p.A52 (2020) |

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Spectral properties and detectability of supermassive stars in protoglobular clusters at high redshift ![]() Author(s): Martins F., Schaerer D., Haemmerlé L., Charbonnel C. (Article) Published: Astronomy & Astrophysics, vol. 633 p.A9 (2020) |

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Massive stars in extremely metal-poor galaxies: A window into the past ![]() Author(s): Garcia M., Evans C.J., Bestenlehner J.M., Bouret J.C., Castro N., Cerviño M., Fullerton A.W., Gieles M., Herrero A., De Koter A., Lennon D.J., van Loon J.Th., Martins F., de Mink S.E., Najarro F., Negueruela I., Sana H., Simón-Díaz S., Szécsi D., Tramper F., Vink J., Wofford A.
(Document without bibliographic reference) Links openAccess full text : |