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Chemical evolution with rotating massive star yields – I. The solar neighbourhood and the s-process elements

Monthly notices of the Royal Astronomical Society, 2018-05, Vol.476 (3), p.3432-3459

2018

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Chemical evolution with rotating massive star yields II. A new assessment of the solar s- and r- process components

Monthly notices of the Royal Astronomical Society, 2020-01, Vol.491, p.1832-1850

2020

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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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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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Uncertainties in s-process nucleosynthesis in low-mass stars determined from Monte Carlo variations

Monthly notices of the Royal Astronomical Society, 2018-08, Vol.478 (3), p.4101-4127

2018

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Optical and near-infrared coverage of SN 2004et: physical parameters and comparison with other Type IIP supernovae

Monthly notices of the Royal Astronomical Society, 2010-05, Vol.404 (2), p.981-1004

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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Chemical evolution with rotating massive star yields II. A new assessment of the solar s- and r-process components

Monthly notices of the Royal Astronomical Society, 2020, Vol.491, p.1832-1850

2020

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The branchings of the main s-process: their sensitivity to alpha -induced reactions on super( 13)C and super( 22)Ne and to the uncertainties of the nuclear network

Monthly notices of the Royal Astronomical Society, 2015-05, Vol.449 (1), p.506-506

2015

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The branchings of the main s-process: their sensitivity to [alpha]-induced reactions on ^sup 13^C and ^sup 22^Ne and to the uncertainties of the nuclear network

Monthly notices of the Royal Astronomical Society, 2015-05, Vol.449 (1), p.506

2015

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The branchings of the main s-process: their sensitivity to α-induced reactions on 13C and 22Ne and to the uncertainties of the nuclear network

Monthly notices of the Royal Astronomical Society, 2015-05, Vol.449 (1), p.506-527

2015

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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: The s-process in low-metallicity stars - III

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

2012

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

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

2011

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

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

2011

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Optical and near-infrared coverage of SN 2004et: physical parameters and comparison with other Type IIP supernovae

Monthly notices of the Royal Astronomical Society, 2010-05, Vol.404 (2), p.981-1004

2010

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Optical and near-infrared coverage of SN 2004et: physical parameters and comparison with other Type IIP supernovae: Optical and NIR coverage of SN 2004et

Monthly notices of the Royal Astronomical Society, 2010-05, Vol.404 (2), p.981-1004

2010

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Chandrasekhar-mass white dwarfs are the progenitors of a small fraction of Type Ia supernovae according to nucleosythesis constraints

Monthly notices of the Royal Astronomical Society. Letters, 2022-11, Vol.517 (1), p.L31-L35

2022

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On the origin of the Galactic thin and thick discs, their abundance gradients and the diagnostic potential of their abundance ratios

Monthly notices of the Royal Astronomical Society, 2023-05, Vol.523 (2), p.2126-2145

2023

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Impact of newly measured 26Al(n, p)26Mg and 26Al(n, α)23Na reaction rates on the nucleosynthesis of 26Al in stars

Monthly notices of the Royal Astronomical Society, 2023-02, Vol.520 (2), p.2436-2444

2023

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He-accreting WD: nucleosynthesis in the extreme binary system (1.02 + 0.30) M

Monthly notices of the Royal Astronomical Society, 2019-03, Vol.484 (1), p.950-963

2019

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Erratum: He-accreting WD: Nucleosynthesis in the extreme binary system (1.02 + 0.30) M

Monthly notices of the Royal Astronomical Society, 2019-06, Vol.486 (1), p.1480-1480

2019

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Apoprotein E polymorphism and microalbuminuria in type 2 diabetic patients

American journal of hypertension, 2003-05, Vol.16 (5), p.A244-A244

2003

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P-568: Apoprotein E polymorphism and microalbuminuria in type 2 diabetic patients

American journal of hypertension, 2003-05, Vol.16 (S1), p.244A-244A

2003

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Chemical evolution with rotating massive star yields – I. The solar neighbourhood and the s-process elements

Chemical evolution with rotating massive star yields II. A new assessment of the solar s- and r- process components

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

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

Uncertainties in s-process nucleosynthesis in low-mass stars determined from Monte Carlo variations

Optical and near-infrared coverage of SN 2004et: physical parameters and comparison with other Type IIP supernovae

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

Chemical evolution with rotating massive star yields II. A new assessment of the solar s- and r-process components

The branchings of the main s-process: their sensitivity to alpha -induced reactions on super( 13)C and super( 22)Ne and to the uncertainties of the nuclear network

The branchings of the main s-process: their sensitivity to [alpha]-induced reactions on ^sup 13^C and ^sup 22^Ne and to the uncertainties of the nuclear network

The branchings of the main s-process: their sensitivity to α-induced reactions on 13C and 22Ne and to the uncertainties of the nuclear network

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

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

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

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

Optical and near-infrared coverage of SN 2004et: physical parameters and comparison with other Type IIP supernovae

Optical and near-infrared coverage of SN 2004et: physical parameters and comparison with other Type IIP supernovae: Optical and NIR coverage of SN 2004et

Chandrasekhar-mass white dwarfs are the progenitors of a small fraction of Type Ia supernovae according to nucleosythesis constraints

On the origin of the Galactic thin and thick discs, their abundance gradients and the diagnostic potential of their abundance ratios

Impact of newly measured 26Al(n, p)26Mg and 26Al(n, α)23Na reaction rates on the nucleosynthesis of 26Al in stars

He-accreting WD: nucleosynthesis in the extreme binary system (1.02 + 0.30) M

Erratum: He-accreting WD: Nucleosynthesis in the extreme binary system (1.02 + 0.30) M

Apoprotein E polymorphism and microalbuminuria in type 2 diabetic patients

P-568: Apoprotein E polymorphism and microalbuminuria in type 2 diabetic patients

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