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Evolution, Nucleosynthesis, and Yields of Low-mass Asymptotic Giant Branch Stars at Different Metallicities. II. The FRUITY Database

The Astrophysical journal. Supplement series, 2011-12, Vol.197 (2), p.17-jQuery1323919387692='48'

2011

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EVOLUTION, NUCLEOSYNTHESIS, AND YIELDS OF AGB STARS AT DIFFERENT METALLICITIES. III. INTERMEDIATE-MASS MODELS, REVISED LOW-MASS MODELS, AND THE pH-FRUITY INTERFACE

The Astrophysical journal. Supplement series, 2015-08, Vol.219 (2), p.1-21

2015

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Evolution, Nucleosynthesis, and Yields of Low-Mass Asymptotic Giant Branch Stars at Different Metallicities

The Astrophysical journal, 2009-05, Vol.696 (1), p.797-820

2009

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The RGB tip of galactic globular clusters and the revision of the axion-electron coupling bound

Astronomy and astrophysics (Berlin), 2020-12, Vol.644, p.A166

2020

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THE EFFECTS OF ROTATION ON s -PROCESS NUCLEOSYNTHESIS IN ASYMPTOTIC GIANT BRANCH STARS

The Astrophysical journal, 2013-09, Vol.774 (2), p.1-11

2013

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HEAVY ELEMENTS IN GLOBULAR CLUSTERS: THE ROLE OF ASYMPTOTIC GIANT BRANCH STARS

The Astrophysical journal, 2014-04, Vol.785 (1), p.1-18

2014

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The s-process in low-metallicity stars - II. Interpretation of high-resolution spectroscopic observations with asymptotic giant branch models

Monthly notices of the Royal Astronomical Society, 2011-11, Vol.418 (1), p.284-319

2011

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Properties of carbon stars in the solar neighbourhood based on Gaia DR2 astrometry

Astronomy and astrophysics (Berlin), 2020-01, Vol.633, p.A135

2020

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The puzzle of the CNO isotope ratios in asymptotic giant branch carbon stars

Astronomy and astrophysics (Berlin), 2017-03, Vol.599, p.A39

2017

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The s-process in low-metallicity stars - III. Individual analysis of CEMP-s and CEMP-s/r with asymptotic giant branch models

Monthly notices of the Royal Astronomical Society, 2012-05, Vol.422 (1), p.849-884

2012

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s-Process in low-metallicity stars – I. Theoretical predictions

Monthly notices of the Royal Astronomical Society, 2010-05, Vol.404 (3), p.1529-1544

2010

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The status and future of direct nuclear reaction measurements for stellar burning

Journal of physics. G, Nuclear and particle physics, 2022-01, Vol.49 (1), p.10501

2022

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First spectroscopic investigation of anomalous Cepheid variables

Astronomy and astrophysics (Berlin), 2024-02, Vol.682, p.A1

2024

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Do we really know Mup (i.e. the transition mass between Type Ia and core-collapse supernova progenitors)?

Journal of physics. Conference series, 2016-01, Vol.665 (1)

2016

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Molecular Opacities for Low-Mass Metal-poor AGB Stars Undergoing the Third Dredge-up

The Astrophysical journal, 2007-09, Vol.667 (1), p.489-496

2007

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Oxygen isotopic ratios in intermediate-mass red giants

Astronomy and astrophysics (Berlin), 2015-06, Vol.578, p.A33

2015

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The Importance of the 13C( ,n)16O Reaction in Asymptotic Giant Branch Stars

The Astrophysical journal, 2018-05, Vol.859 (2)

2018

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Deep FORS1 Observations of the Double Main Sequence of ω Centauri

The Astrophysical journal, 2007-01, Vol.654 (2), p.915-922

2007

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NITROGEN ISOTOPES IN ASYMPTOTIC GIANT BRANCH CARBON STARS AND PRESOLAR SiC GRAINS: A CHALLENGE FOR STELLAR NUCLEOSYNTHESIS

Astrophysical journal. Letters, 2013-05, Vol.768 (1), p.1-5

2013

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The O-Na and Mg-Al anticorrelations in turn-off and early subgiants in globular clusters

Astronomy and astrophysics (Berlin), 2001-04, Vol.369 (1), p.87-98

2001

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Do we really know M up (i.e. the transition mass between Type Ia and core-collapse supernova progenitors)?

Journal of physics. Conference series, 2016, Vol.665, p.12008

2016

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A method to derive the absolute composition of the Sun, the solar system, and the stars

Astronomy and astrophysics (Berlin), 2007-02, Vol.462 (3), p.1051-1062

2007

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Metallicity as a Source of Dispersion in the SNIa Bolometric Light Curve Luminosity-Width Relationship

Astrophysical journal. Letters, 2010-03, Vol.711 (2), p.L66-L70

2010

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NGC 1866: a milestone for understanding the chemical evolution of stellar populations in the Large Magellanic Cloud

Monthly notices of the Royal Astronomical Society, 2011-05, Vol.413 (2), p.837-851

2011

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Very low-mass white dwarfs with a C–O core

Astronomy and astrophysics (Berlin), 2009-12, Vol.507 (3), p.1575-1583

2009

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Evolution, Nucleosynthesis, and Yields of Low-mass Asymptotic Giant Branch Stars at Different Metallicities. II. The FRUITY Database

EVOLUTION, NUCLEOSYNTHESIS, AND YIELDS OF AGB STARS AT DIFFERENT METALLICITIES. III. INTERMEDIATE-MASS MODELS, REVISED LOW-MASS MODELS, AND THE pH-FRUITY INTERFACE

Evolution, Nucleosynthesis, and Yields of Low-Mass Asymptotic Giant Branch Stars at Different Metallicities

The RGB tip of galactic globular clusters and the revision of the axion-electron coupling bound

THE EFFECTS OF ROTATION ON s -PROCESS NUCLEOSYNTHESIS IN ASYMPTOTIC GIANT BRANCH STARS

HEAVY ELEMENTS IN GLOBULAR CLUSTERS: THE ROLE OF ASYMPTOTIC GIANT BRANCH STARS

The s-process in low-metallicity stars - II. Interpretation of high-resolution spectroscopic observations with asymptotic giant branch models

Properties of carbon stars in the solar neighbourhood based on Gaia DR2 astrometry

The puzzle of the CNO isotope ratios in asymptotic giant branch carbon stars

The s-process in low-metallicity stars - III. Individual analysis of CEMP-s and CEMP-s/r with asymptotic giant branch models

s-Process in low-metallicity stars – I. Theoretical predictions

The status and future of direct nuclear reaction measurements for stellar burning

First spectroscopic investigation of anomalous Cepheid variables

Do we really know Mup (i.e. the transition mass between Type Ia and core-collapse supernova progenitors)?

Molecular Opacities for Low-Mass Metal-poor AGB Stars Undergoing the Third Dredge-up

Oxygen isotopic ratios in intermediate-mass red giants

The Importance of the 13C( ,n)16O Reaction in Asymptotic Giant Branch Stars

Deep FORS1 Observations of the Double Main Sequence of ω Centauri

NITROGEN ISOTOPES IN ASYMPTOTIC GIANT BRANCH CARBON STARS AND PRESOLAR SiC GRAINS: A CHALLENGE FOR STELLAR NUCLEOSYNTHESIS

The O-Na and Mg-Al anticorrelations in turn-off and early subgiants in globular clusters

Do we really know M up (i.e. the transition mass between Type Ia and core-collapse supernova progenitors)?

A method to derive the absolute composition of the Sun, the solar system, and the stars

Metallicity as a Source of Dispersion in the SNIa Bolometric Light Curve Luminosity-Width Relationship

NGC 1866: a milestone for understanding the chemical evolution of stellar populations in the Large Magellanic Cloud

Very low-mass white dwarfs with a C–O core

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