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Published in Galaxies (01.02.2023)
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Published in Proceedings of the International Astronomical Union (01.07.2010)
Published in Proceedings of the International Astronomical Union (01.07.2010)
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Published in Proceedings of the International Astronomical Union (01.07.2010)
Published in Proceedings of the International Astronomical Union (01.07.2010)
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Near-infrared Spectra of a Sample of Galactic Unclassified B[e] Stars Based on observations obtained at (1) the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), Ministério da Ciência, Tecnologia e Inovação (Brazi
Arias, María L., Cidale, Lydia S., Kraus, Michaela, Torres, Andrea F., Aidelman, Yael, Zorec, Juan, Granada, Anahí
Published in Publications of the Astronomical Society of the Pacific (02.10.2018)
Published in Publications of the Astronomical Society of the Pacific (02.10.2018)
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Published in arXiv.org (07.03.2013)
Published in arXiv.org (07.03.2013)
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Populations of rotating stars. - I. Models from 1.7 to 15 Msun at Z = 0.014, 0.006, and 0.002 with {\Omega}/{\Omega}crit between 0 and 1
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Published in arXiv.org (10.03.2013)
Published in arXiv.org (10.03.2013)
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Georgy, Cyril, Ekström, Sylvia, Saio, Hideyuki, Meynet, Georges, Groh, Jose, Granada, Anahí
Published in arXiv.org (07.03.2013)
Published in arXiv.org (07.03.2013)
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Massive stellar models: rotational evolution, metallicity effects
Ekström, Sylvia, Georgy, Cyril, Meynet, Georges, Maeder, André, Granada, Anahí
Published in arXiv.org (19.10.2010)
Published in arXiv.org (19.10.2010)
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Radiation driven winds with rotation: The oblate finite disc correction factor
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Grids of stellar models with rotation - III. Models from 0.8 to 120 Msun at a metallicity Z = 0.002
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Published in arXiv.org (23.08.2013)
Published in arXiv.org (23.08.2013)
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Grids of stellar models with rotation - I. Models from 0.8 to 120 Msun at solar metallicity (Z = 0.014)
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Published in arXiv.org (21.11.2011)
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Published in Proceedings of the International Astronomical Union (01.12.2011)
Published in Proceedings of the International Astronomical Union (01.12.2011)
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Published in Proceedings of the International Astronomical Union (01.12.2010)
Published in Proceedings of the International Astronomical Union (01.12.2010)
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Populations of rotating stars III. SYCLIST, the new Geneva Population Synthesis code
Georgy, Cyril, Granada, Anahi, Ekström, Sylvia, Meynet, Georges, Anderson, Richard I, Wyttenbach, Aurélien, Eggenberger, Patrick, Maeder, André
Published in arXiv.org (28.04.2014)
Published in arXiv.org (28.04.2014)
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