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We explore the consequences of an early population of intermediate mass stars in the 2 - 8 M\odot range on cosmic chemical evolution. We discuss the implications of this population as it pertains to s...
Models of primordial and hyper-metal-poor stars with masses similar to the Sun experience an ingestion of protons into the hot core during the core helium flash phase at the end of their red giant bra...
Energy in stars is provided by nuclear reactions, which, in many cases, produce radioactive nuclei. When stable nuclei are irradiated by a flux of protons or neutrons, capture reactions push stable ma...
The delayed contribution of low and intermediate mass stars to chemical galactic enrichment:an analytical approach。
Evidence for rotation-induced mixing in evolved intermediate mass stars
Accretion in young low intermediate mass stars
Parsec-Scale Outflows from Intermediate-Mass Stars
The evolution of intermediate mass stars from the main sequence to the white dwarf stage。

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