摘要
介绍和评述了有关星际26Al问题的各种新星模型计算结果，阐述了我们对这一问题的研究和看法，指出了现今各种新星模型在星际26Al问题上存在的严重困难。
The results of various models of novae for thc origin of the interstellar 26Al are reviewed. A constraint on the abundance ratio X(22Na)/X(26Al) produced by novaeis discussed, based on the observation from space. The conclusion is that all the nova models up to now are hard to provide enough detected interstellar 26Al.
出处
《天文学进展》
CSCD
北大核心
1995年第4期305-314,共10页
Progress In Astronomy
基金
国家八五攀登计划资助
国家自然科学基金
