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The impact of the uncertainties in the 12C(α, γ)16O reaction rate on the evolution of low- to intermediate-mass stars
Ben T Pepper, A G Istrate, A D Romero and S O Kepler Monthly Notices of the Royal Astronomical Society 513(1) 1499 (2022) https://doi.org/10.1093/mnras/stac1016
Hints of the Existence of C-rich Massive Evolved Stars∗
Guillermo Quintana-Lacaci, José Cernicharo, Marcelino Agúndez, José Pablo Fonfría, Luis Velilla-Prieto, Carmen Sánchez Contreras, Valentín Bujarrabal, Arancha Castro-Carrizo and Javier Alcolea The Astrophysical Journal 876(2) 116 (2019) https://doi.org/10.3847/1538-4357/ab133e
The VIMOS Ultra Deep Survey: Nature, ISM properties, and ionizing spectra of CIII]λ1909 emitters at z = 2–4
A test for asymptotic giant branch evolution theories: planetary nebulae in the Large Magellanic Cloud
P. Ventura, L. Stanghellini, F. Dell'Agli, D. A. García-Hernández and M. Di Criscienzo Monthly Notices of the Royal Astronomical Society 452(4) 3679 (2015) https://doi.org/10.1093/mnras/stv1590
CAN STAR CLUSTER ENVIRONMENT AFFECT DUST INPUT FROM MASSIVE AGB STARS?
The effect of including molecular opacities of variable composition on the evolution of intermediate-mass AGB stars
C. K. Fishlock, A. I. Karakas and R. J. Stancliffe Monthly Notices of the Royal Astronomical Society 438(2) 1741 (2014) https://doi.org/10.1093/mnras/stt2313
ON THE NECESSITY OF COMPOSITION-DEPENDENT LOW-TEMPERATURE OPACITY IN MODELS OF METAL-POOR ASYMPTOTIC GIANT BRANCH STARS
Evolution of thermally pulsing asymptotic giant branch stars – I. The colibri code
Paola Marigo, Alessandro Bressan, Ambra Nanni, Léo Girardi and Maria Letizia Pumo Monthly Notices of the Royal Astronomical Society 434(1) 488 (2013) https://doi.org/10.1093/mnras/stt1034
Dust input from AGB stars in the Large Magellanic Cloud
Francesca D'Antona, Corinne Charbonnel, Wojciech Dziembowski, et al. Proceedings of the International Astronomical Union 4(T27A) 211 (2008) https://doi.org/10.1017/S1743921308025544
Bayesian posterior classification of planetary nebulae according to the Peimbert types