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Very Massive Stars: Near and Far.
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- Proceedings of the International Astronomical Union, 2024, v. 18, n. S361, p. 369, doi. 10.1017/S1743921322002149
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Very Massive Stars: Near and Far.
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- Proceedings of the International Astronomical Union, 2022, v. 18, n. S361, p. 369, doi. 10.1017/S1743921322002149
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Understanding structure in line-driven stellar winds using ultraviolet spectropolarimetry in the time domain.
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- Astrophysics & Space Science, 2022, v. 367, n. 12, p. 1, doi. 10.1007/s10509-022-04142-6
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Star-planet interactions: IV. Possibility of detecting the orbit-shrinking of a planet around a red giant.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2017, v. 602, p. 1, doi. 10.1051/0004-6361/201730999
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Evolution of surface CNO abundances in massive stars.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2014, v. 566, p. 1, doi. 10.1051/0004-6361/201220602
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On the effect of rotation on populations of classical Cepheids I. Predictions at solar metallicity.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2014, v. 564, p. 1, doi. 10.1051/0004-6361/201322988
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The evolution of massive stars and their spectra I. A non-rotating 60 M☉ star from the zero-age main sequence to the pre-supernova stage.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2014, v. 564, p. 1, doi. 10.1051/0004-6361/201322573
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Progenitors of supernova Ibc: a single Wolf-Rayet star as the possible progenitor of the SN Ib iPTF13bvn.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2013, v. 558, p. 1, doi. 10.1051/0004-6361/201322369
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Fundamental properties of core-collapse supernova and GRB progenitors: predicting the look of massive stars before death.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2013, v. 558, p. 1, doi. 10.1051/0004-6361/201321906
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What Young Massive Clusters in the Magellanic Clouds teach us about Old Galactic Globular Clusters?
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- Proceedings of the International Astronomical Union, 2018, v. 14, n. S343, p. 314, doi. 10.1017/S174392131800563X
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Massive star evolution: feedbacks in low- Z environment.
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- Proceedings of the International Astronomical Union, 2018, v. 14, n. S344, p. 153, doi. 10.1017/S1743921318007238
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Massive stars: stellar models and stellar yields, impact on Galactic Archaeology.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S334, p. 170, doi. 10.1017/S1743921317010808
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Massive stars, successes and challenges.
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- Proceedings of the International Astronomical Union, 2016, v. 12, n. S329, p. 3, doi. 10.1017/S1743921317003283
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Synthetic clusters of massive stars to test stellar evolution models.
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- Proceedings of the International Astronomical Union, 2015, v. 12, n. S316, p. 355, doi. 10.1017/S1743921315008868
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The luminosity distribution of RSGs to test their mass-loss rate.
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- Proceedings of the International Astronomical Union, 2015, v. 11, n. A29B, p. 454, doi. 10.1017/S1743921316005809
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Rotation and the Cepheid Mass Discrepancy.
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- Proceedings of the International Astronomical Union, 2014, v. 9, n. S307, p. 206, doi. 10.1017/S1743921314006723
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Population synthesis at the crossroads.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S284, p. 2, doi. 10.1017/S1743921312008605
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Theoretical stellar ΔY/ΔO in the early Universe.
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- Proceedings of the International Astronomical Union, 2009, v. 5, n. S268, p. 447, doi. 10.1017/S1743921310004618
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The basic role of magnetic fields in stellar evolution.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S259, p. 311, doi. 10.1017/S1743921309030671
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Stellar evolution models at the Magellanic Cloud metallicities.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S256, p. 337, doi. 10.1017/S1743921308028676
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Stellar Evolution in the Early Universe.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S255, p. 297, doi. 10.1017/S1743921308024976
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Powerful explosions at Z = 0?
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S255, p. 194, doi. 10.1017/S1743921308024812
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Evolution and chemical and dynamical effects of high-mass stars.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S254, p. 325, doi. 10.1017/S1743921308027774
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Massive star evolution: from the early to the present day Universe.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S252, p. 317, doi. 10.1017/S1743921308023119
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Stellar Evolution at Low Metallicity.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S250, p. 217, doi. 10.1017/S1743921308020528
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Can Very Massive Stars Avoid Pair-Instability Supernovae?
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S250, p. 209, doi. 10.1017/S1743921308020516
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Developments in Physics of Massive Stars.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S250, p. 147, doi. 10.1017/S1743921308020449
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Massive Stars as Cosmic Engines Through the Ages.
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- Proceedings of the International Astronomical Union, 2007, v. 3, n. S250, p. 3, doi. 10.1017/S1743921308020292
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Fast rotating first stars.
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- Proceedings of the International Astronomical Union, 2005, v. 1, n. S228, p. 163, doi. 10.1017/S174392130500548X
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Rapidly rotating Population III stellar models as a source of primary nitrogen.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 687, p. 1, doi. 10.1051/0004-6361/202449156
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Pre-supernova mixing in CEMP-no source stars.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2017, v. 605, p. 1, doi. 10.1051/0004-6361/201630182
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- Article