FIRST STARS FORMATION WITH THE PRESENCE OF A PRIMORDIAL MAGNETIC FIELD

被引：0
|
作者：
Nunez-Lopez, R. [1 ]
Lipovka, A. [1 ]
机构：
[1] Univ Sonora, Dept Invest Fis, Hermosillo 83000, Sonora, Mexico
来源：
XIII LATIN AMERICAN REGIONAL IAU MEETING | 2011年 / 40卷
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D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The problem of the metal-free Pop III stars cooling is considered. The importance of the cyclotron cooling in the presence of the primordial magnetic field is discussed. It is shown that the cyclotron cooling must be taken into account as well as cooling due to H-2, HD and LiH molecules.
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页码：25 / 25
页数：1
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