搜索结果: 1-8 共查到“理学 Intermediate-Mass Stars”相关记录8条 . 查询时间(0.123 秒)
Cosmic Chemical Evolution with an Early Population of Intermediate Mass Stars
Cosmic Chemical Evolution Intermediate Mass Stars
2011/1/11
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...
Evolution and nucleosynthesis of extremely metal-poor and metal-free low- and intermediate-mass stars II. s-process nucleosynthesis during the core He flash
Solar and Stellar Astrophysics (astro-ph.SR)
2010/12/28
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...
Radioactivities in Low- and Intermediate-Mass Stars
Solar and Stellar Astrophysics (astro-ph.SR)
2010/12/27
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
stars analytical approach chemical galactic enrichment
2009/7/10
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
rotation-induced mass stars
2009/6/25
Evidence for rotation-induced mixing in evolved intermediate mass stars。
Accretion in young low intermediate mass stars。
Parsec-Scale Outflows from Intermediate-Mass Stars
Parsec-Scale Outflows Intermediate-Mass Stars
2009/6/15
Parsec-Scale Outflows from Intermediate-Mass Stars。
The evolution of intermediate mass stars from the main sequence to the white dwarf stage
mass stars white dwarf stage main sequence
2009/6/10
The evolution of intermediate mass stars from the main sequence to the white dwarf stage。