非爆�性氢燃烧：我们目前所处的阶段如何？
天体物理学
2007-05-23 v1
摘要
讨论了核物理不确定性对冷CNO、NeNa和MgAl型稳态氢燃烧模式下预测产物丰度的影响。除了能够定性地模拟详细星体模型的预测外，这些参数化计算还具有一种纯粹核物理来源丰度不确定性的清晰分离优势。
引用
@article{arxiv.astro-ph/9512027,
title = {Non-Explosive Hydrogen Burning: Where Do We Stand?},
author = {M. Arnould and N. Mowlavi and A. Champagne},
journal= {arXiv preprint arXiv:astro-ph/9512027},
year = {2007}
}
备注
13 pages, ps file (gziped + uuencoded), figures included. Review paper presented at the 32nd Liege Int. Astroph. Coll., "Stellar evolution: What Should Be Done?"