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Computational perspective on structure, energetics, and bonding of FeC<sub>2</sub>O isomers with astrochemical significance. [PDF]
Front ChemR J A, Rajasabai SP.
europepmc +1 more source
Photon strength functions and nuclear level densities: invaluable input for nucleosynthesis. [PDF]
Philos Trans A Math Phys Eng SciWiedeking M, Goriely S.
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Asymptotic giant branch and super-asymptotic giant branch stars: modelling dust production at solar metallicity [PDF]
Monthly Notices of the Royal Astronomical Society, 2017 We present dust yields for asymptotic giant branch (AGB) and super-asymptotic giant branch (SAGB) stars of solar metallicity. Stars with initial mass 1.5 M⊙ ≤ Mini ≤ 3 M⊙ reach the carbon star stage during the AGB phase and produce mainly solid carbon ...
Raffaella Schneider +2 more
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Mixing and Magnetic Fields in Asymptotic Giant Branch Stars in the Framework of FRUITY Models
Universe, 2022Diego Vescovi
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s-Processing in Asymptotic Giant Branch Stars in the Light of Revised Neutron-Capture Cross Sections
Universe, 2021Rene Reifarth, Diego Vescovi
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Evolution of Asymptotic Giant Branch Stars
Annual Review of Astronomy and Astrophysics, 2005Falk Herwig
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Observations and Modelling of Spectral Energy Distributions of Asymptotic Giant Branch Stars
Astrophysics and Space Science, 1997J G Doyle, J G Doyle
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