Heartbeats of a neutron star

被引：0
|
作者：
Robert V. Wagoner
机构：
[1] Stanford University,the Department of Physics
来源：
Nature | 2003年 / 424卷
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摘要：
Different oscillations in the flux of X-rays emitted from a neutron star now seem to be linked to the frequency at which the star is spinning. That spin rate in turn hints at what the interior of such a star is made of.
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页码：27 / 28
页数：1
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