The galactic dark matter: Predictions and observations

被引：0
作者：
Oldershaw R.L. [1 ]
机构：
[1] Amherst College (Box 2262), Amherst
来源：
Astrophysics and Space Science | 1997年 / 257卷 / 2期
关键词：
Black Hole; Dark Matter; Cosmological Model; Cold Dark Matter; Dark Matter Mass;
D O I：
10.1023/A:1001108212691
中图分类号：
学科分类号：
摘要：
After two decades of efforts to identify the enigmatic dark matter that comprises the dominant form of matter in our galaxy, the mass range for viable candidates appears to have been reduced by more than 50 orders of magnitude. Positive results have thus far been confined to the range: 10-7 M⊙ to 1.0 M⊙, with apparent clustering within the ranges 10-5 M⊙ to 10-3 M⊙ and 0.08 M⊙ to 0.5 M⊙. Positive and negative results are compared with specific predictions of cosmological models.
引用
收藏
页码：271 / 278
页数：7
相关论文
共 44 条
[1]  
Adams F.C., Laughlin G., Astrophys. J., (1996)
[2]  
Alcock C., Akerlof C.W., Allsman R.A., Et al., Nature, 365, (1993)
[3]  
Alcock C., Allsman R.A., Axelrod T.S., Et al., Astrophys. J., 461, (1996)
[4]  
Alcock C., Allsman R.A., Alves D., Et al., Astrophys. J., 471, (1996)
[5]  
Ashman K.M., Publ. Astron. Soc. Pacific, 104, (1992)
[6]  
Aubourg E., Bareyre P., Brehin S., Et al., Nature, 365, (1993)
[7]  
Bennett D., Et al., Proceedings of 'Planets Beyond the Solar System and the Next Generation of Space Missions', (1996)
[8]  
Canal R., Isern J., Ruiz-Lapuente P., Astrophys. J., 488, (1997)
[9]  
Carr B.J., Annu. Rev. Astron. Astrophys., 32, (1994)
[10]  
Cummings C.M., De Robertis M.M., Publ. Astron. Soc. Pacific, 107, (1995)
12345