摘要
利用银河系三成分(晕、厚盘和薄盘)星系化学演化模型,在比较了计算结果和可观测量的基础上,得出:Ⅰa型超新星数目约占恒星总数目的0.03。
Use the chemical evolution model of three-zone(the halo thick disk and thin disk),on the basis of compared the theoretical calculation and the observational constrains, it is shown that the number of type I a supernova is 3 percent of the whole milk-way galaxiy stellars.
出处
《沧州师范学院学报》
2007年第3期37-38,共2页
Journal of Cangzhou Normal University
关键词
元素丰度
星系演化模型
观测约束
Element abundance
Galactic chemical evolution model
observational constrains.