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https://www.academia.edu/75227803/Infrared_Photometry_and_Evolution_of_Mass_Losing_AGB_Stars_II_Luminosity_and_Colors_of_MS_and_S_Stars
(PDF) Infrared Photometry and Evolution of Mass-Losing AGB Stars. II. Luminosity and Colors of MS...
AGB phases mark the end of the evolution for Low- and Intermediate-Mass Stars. Our understanding of the mechanisms through which they eject the envelope and...
agb starspdfinfraredphotometryevolution
https://www.academia.edu/81691348/Low_mass_lithium_rich_AGB_stars_in_the_Galactic_bulge_evidence_for_cool_bottom_processing
(PDF) Low-mass lithium-rich AGB stars in the Galactic bulge: evidence for cool bottom processing?
Context. The stellar production of the light element lithium is still a matter of debate. Aims. We report the detection of low-mass, Li-rich Asymptotic Giant...
pdf lowagb starsmasslithiumrich
https://www.academia.edu/66410285/Extra_mixing_in_AGB_Stars_from_magnetic_buoyancy
(PDF) Extra-mixing in AGB Stars from magnetic buoyancy
We study the circulation of matter in AGB stars above the H-burning shell, which is known to yield the appearance of p-rich isotopes like 13C, 17O and the...
pdf extraagb starsmixingmagneticbuoyancy
https://www.academia.edu/66409963/Technetium_and_the_third_dredge_up_in_AGB_stars
(PDF) Technetium and the third dredge up in AGB stars
Context. Technetium (Tc) is an unstable element synthesised via the s-process in deep layers of asymptotic giant branch (AGB) stars, making it a reliable...
agb starspdftechnetiumthirddredge