Pulsation in Intermediate-Mass Stars
نویسندگان
چکیده
منابع مشابه
Nucleosynthesis in Intermediate Mass Stars
We discuss nucleosynthesis within 6 M models with Z = 0:02, 0:008 and 0:004. The emphasis is on the AGB phase of evolution, with particular reference to thermal pulses and Hot Bottom Burning. We nd strong CN cycling, with substantial Al production, especially at low metallicities.
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ژورنال
عنوان ژورنال: Frontiers in Astronomy and Space Sciences
سال: 2018
ISSN: 2296-987X
DOI: 10.3389/fspas.2018.00043