Relativistic beaming and quasar statistics

Relativistic beaming and quasar statistics
复制标题

DOI:
10.1093/mnras/200.4.1067
复制
发表时间:
1982-10
影响因子:
4.8
通讯作者:
M. J. L. Orr;I. W. A. Browne
M. J. L. Orr;I. W. A. Browne
中科院分区:
物理与天体物理2区
文献类型:
--
作者:
M. J. L. Orr;I. W. A. Browne

文献摘要

被引文献

相似文献

一个计划的预测属性之间的平坦和陡峭的光谱类星体的投影和相对论性聚束的影响进行了探讨。我们的结论是,类星体的统计性质是完全符合这样的方案提供的平均洛伦兹因子在类星体的中心组件是~5。
The predictions of a scheme which attributes the observed differences between flat and steep spectrum quasars to projection and the effects of relativistic beaming are explored. We conclude that the statistical properties of quasars are entirely consistent with such a scheme provided the mean Lorentz factor in the central components of quasars is ~5.