Synthesis of Organic and Inorganic Compounds in Asymptotic Giant Branch Stars
After the synthesis of carbon in the core of asymptotic giant branch (AGB) stars, carbon is dredged up to the surface by convection. Many carbon-based molecules are formed in the subsequently developed stellar wind.
Sun Kwok
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The brightest asymptotic giant branch stars in the Leo I dwarf spheroidal galaxy [PDF]
J. W. Menzies+4 more
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The precise definition of the lower mass limit of red supergiant stars (RSGs) is an open question in astrophysics and does not attract much attention.
Ming Yang+10 more
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Evidence of structural discontinuities in the inner core of red-giant stars. [PDF]
Vrard M+5 more
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A Chemical Route to the Formation of Water in the Circumstellar Envelopes around Carbon-rich Asymptotic Giant Branch Stars: Fischer-Tropsch Catalysis [PDF]
Karen Willacy
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Chemical enrichment by Wolf--Rayet and asymptotic giant branch stars [PDF]
Lynnette Dray+3 more
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On Titanium Carbide Nanoparticles as the Origin of the 21 Micron Emission Feature in Post-asymptotic Giant Branch Stars [PDF]
Aigen Li
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Simulations of Solar and Stellar Dynamos and Their Theoretical Interpretation. [PDF]
Käpylä PJ+4 more
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Neutral Carbon in Post–Asymptotic Giant Branch Stars and Planetary Nebulae [PDF]
T. Hasegawa, Sun Kwok
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