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Presolar Grain Isotopic Ratios as Constraints to Nuclear and Stellar Parameters of Asymptotic Giant Branch Star Nucleosynthesis
Sara Palmerini, Maurizio Busso, Diego Vescovi, Eugenia Naselli, Angelo Pidatella, Riccardo Mucciola, Sergio Cristallo, David Mascali, Alberto Mengoni, Stefano Simonucci and Simone Taioli The Astrophysical Journal 921(1) 7 (2021) https://doi.org/10.3847/1538-4357/ac1786
Duncan K. Galloway and Laurens Keek 461 209 (2021) https://doi.org/10.1007/978-3-662-62110-3_5
The most metal-rich stars in the universe: chemical contributions of low- and intermediate-mass asymptotic giant branch stars with metallicities within 0.04 ≤ Z ≤ 0.10
Carbon–Oxygen Classical Novae Are Galactic 7Li Producers as well as Potential Supernova Ia Progenitors
Sumner Starrfield, Maitrayee Bose, Christian Iliadis, W. Raphael Hix, Charles E. Woodward and R. Mark Wagner The Astrophysical Journal 895(1) 70 (2020) https://doi.org/10.3847/1538-4357/ab8d23
Gamma-ray observations of Nova Sgr 2015 No. 2 with INTEGRAL
Primordial to extremely metal-poor AGB and Super-AGB stars: White dwarf or supernova progenitors?
Pilar Gil-Pons, Carolyn L. Doherty, Jordi L. Gutiérrez, et al. Publications of the Astronomical Society of Australia 35 (2018) https://doi.org/10.1017/pasa.2018.42
The thermal stability of helium burning on accreting neutron stars
Michael Zamfir, Andrew Cumming and Caroline Niquette Monthly Notices of the Royal Astronomical Society 445(3) 3278 (2014) https://doi.org/10.1093/mnras/stu1927
The accretion of solar material onto white dwarfs: No mixing with core material implies that the mass of the white dwarf is increasing