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Nucleosynthesis in stars: The Origin of the Heaviest Elements.
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- Proceedings of the International Astronomical Union, 2018, v. 14, n. S343, p. 79, doi. 10.1017/S1743921318006166
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- Article
The composition of Barium stars and the s-process in AGB stars.
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- Proceedings of the International Astronomical Union, 2018, v. 14, n. S343, p. 89, doi. 10.1017/S1743921318005100
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- Article
On the circumstellar effects on the Li and Ca abundances in massive Galactic O-rich AGB stars.
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- Proceedings of the International Astronomical Union, 2018, v. 14, n. S343, p. 489, doi. 10.1017/S174392131800501X
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- Article
Short-lived radioactivity in the early solar system: The Super-AGB star hypothesis.
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- Meteoritics & Planetary Science, 2012, v. 47, n. 12, p. 1998, doi. 10.1111/j.1945-5100.2012.01411.x
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The role of massive AGB stars in the early solar system composition.
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- Meteoritics & Planetary Science, 2009, v. 44, n. 5, p. 627, doi. 10.1111/j.1945-5100.2009.tb00758.x
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- Article
Effective reduction of graphene oxide using sulfur dioxide-containing chemical compounds.
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- International Journal of Environmental Science & Technology (IJEST), 2019, v. 16, n. 12, p. 8329, doi. 10.1007/s13762-019-02419-y
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- Article
Two distinct sequences of blue straggler stars in the globular cluster M 30.
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- Nature, 2009, v. 462, n. 7276, p. 1028, doi. 10.1038/nature08607
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Determination of Pathogenicity of Bacteria Isolated from Some Aquatic Amphibian and Reptile Species.
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- Biology Bulletin, 2024, v. 51, n. 4, p. 932, doi. 10.1134/S1062359024604725
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- Article
Parametrizing Arf numerical semigroups.
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- Journal of Algebra & Its Applications, 2017, v. 16, n. 11, p. -1, doi. 10.1142/S0219498817502097
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- Article
The GALAH Survey: non-LTE departure coefficients for large spectroscopic surveys.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2020, v. 642, p. 1, doi. 10.1051/0004-6361/202038650
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- Article
Exploring circumstellar effects on the lithium and calcium abundances in massive Galactic O-rich AGB stars.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 623, p. N.PAG, doi. 10.1051/0004-6361/201834611
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- Article
Detailed homogeneous abundance studies of 14 Galactic s-process enriched post-AGB stars: In search of lead (Pb).
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2016, v. 587, p. 1, doi. 10.1051/0004-6361/201527430
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Modelling the observed properties of carbon-enhanced metal-poor stars using binary population synthesis.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2015, v. 581, p. 1, doi. 10.1051/0004-6361/201526200
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- Article
Carbon-enhanced metal-poor stars: a window on AGB nucleosynthesis and binary evolution.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2015, v. 581, p. 1, doi. 10.1051/0004-6361/201525876
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AGB NUCLEOSYNTHESIS AT LOW METALLICITY: WHAT CAN WE LEARN FROM CARBON- AND S-ELEMENTS-ENHANCED METAL-POOR STARS.
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- EAS Publications Series, 2013, v. 64, p. 135, doi. 10.1051/eas/1364019
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The Dawes Review 2: Nucleosynthesis and Stellar Yields of Low- and Intermediate-Mass Single Stars.
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- Publications of the Astronomical Society of Australia, 2014, v. 31, p. N.PAG, doi. 10.1017/pasa.2014.21
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Optimum Design of Braced Steel Space Frames including Soil-Structure Interaction via Teaching-Learning-Based Optimization and Harmony Search Algorithms.
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- Advances in Civil Engineering, 2018, p. 1, doi. 10.1155/2018/3854620
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- Article
The Enigmatic Origins of Li in Sun-like Stars.
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- Resonance: Journal of Science Education, 2020, v. 25, n. 8, p. 1165, doi. 10.1007/s12045-020-1032-9
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The lead discrepancy in intrinsically s-process enriched post-AGB stars in the Magellanic Clouds.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2014, v. 563, p. 1, doi. 10.1051/0004-6361/201323212
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LTE or non-LTE, that is the question The NLTE chemical evolution of strontium in extremely metal-poor stars.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2013, v. 551, p. 1, doi. 10.1051/0004-6361/201220584
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The remarkable solar twin HIP 56948: a prime target in the quest for other Earths.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2012, v. 543, n. 1, p. 1, doi. 10.1051/0004-6361/201117222
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Post-AGB stars in the SMC as tracers of stellar evolution: the extreme s-process enrichment of the 21 μm star J004441.04-732136.4.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2012, v. 541, p. 1, doi. 10.1051/0004-6361/201219150
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Wettability of tundish periclase lining by steel.
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- Refractories & Industrial Ceramics, 2006, v. 47, n. 1, p. 68, doi. 10.1007/s11148-006-0057-2
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Stellar yields – theory and observations.
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- Proceedings of the International Astronomical Union, 2015, v. 11, n. A29B, p. 162, doi. 10.1017/S1743921316004713
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The Chemical Evolution of Heavy Elements in Globular Clusters.
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- Proceedings of the International Astronomical Union, 2013, v. 9, n. S298, p. 439, doi. 10.1017/S1743921313007059
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Stellar yields for chemical evolution modelling.
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- Proceedings of the International Astronomical Union, 2013, v. 9, n. S298, p. 142, doi. 10.1017/S1743921313006315
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- Article
The curious conundrum regarding sulfur and oxygen abundances in planetary nebulae.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S283, p. 384, doi. 10.1017/S1743921312011544
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Heavy elements in planetary nebulae: A theorist's gold mine.
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- Proceedings of the International Astronomical Union, 2011, v. 7, n. S283, p. 127, doi. 10.1017/S1743921312010824
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Globular cluster abundances: the role of asymptotic giant branch stars.
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- Proceedings of the International Astronomical Union, 2009, v. 5, n. S266, p. 161, doi. 10.1017/S1743921309991013
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Chemical abundances in tidally disrupted globular clusters.
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- Proceedings of the International Astronomical Union, 2009, v. 5, n. S266, p. 157, doi. 10.1017/S1743921309991001
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The slow-neutron capture process in low-metallicity asymptotic giant branch stars.
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- Proceedings of the International Astronomical Union, 2009, v. 5, n. S265, p. 57, doi. 10.1017/S1743921310000165
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Insights into the s-process and r-process as revealed by globular clusters.
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- Proceedings of the International Astronomical Union, 2009, v. 5, n. S265, p. 54, doi. 10.1017/S1743921310000153
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