相关实验视频
Updated: Mar 17, 2026

10:17
20 mJ, 1 ps Yb:YAG Thin-disk Regenerative Amplifier
Published on: July 12, 2017
12.1K
一颗无线电脉冲的白矮星
T R Marsh1, B T Gänsicke1, S Hümmerich2,3
1Department of Physics, Gibbet Hill Road, University of Warwick, Coventry CV4 7AL, UK.
Nature
|July 28, 2016
概括
我们发现了AR Scorpii, 一个独特的白矮星双星系统, 这颗磁性白矮星
科学领域:
- * 天文学与天体物理学
- * 紧的星星
- * 二进制系统
背景情况:
- *白矮星是地球大小,密集的恒星残留物.
- * 通常会发射紫外线到近红外线辐射.
- * 在二进制星系中,质量转移可以引起X射线和红外辐射,但远红外/无线电检测很少.
研究的目的:
- 报道发现一颗从X射线到无线电波长发射的白矮星/冷恒星.
- * 描述AR Scorpii系统的不同寻常的发射特性.
主要方法:
- * 多波长观测 (X射线到无线电).
- * 分析光线曲线和光谱特性.
- * 轨道和旋转周期的确定
主要成果:
- *发现AR Scorpii,一个周期为3.56小时的二进制星系.
- 在光学和无线电频率中检测到强烈的快速脉冲 (周期为1.97分钟).
- * 白矮星的倒转功率明显超过电磁输出,表明旋转功率占主导地位.
- * 宽带频谱与同步辐射一致,需要相对论电子.
结论:
- * AR Scorpii是一个主要由自旋驱动的磁性白矮星双星.
- * 由白矮星旋转驱动的脉冲主要来自冷的伴星.
- * 相对论电子对于所观察到的同步子发射至关重要,可能在白矮星附近或在M恒星产生.
相关概念视频
Doppler Effect - II
5.0K
The Doppler effect has several practical, real-world applications. For instance, meteorologists use Doppler radars to interpret weather events based on the Doppler effect. Typically, a transmitter emits radio waves at a specific frequency toward the sky from a weather station. The radio waves bounce off the clouds and precipitation and travel back to the weather station. The radio frequency of the waves reflected back to the station appears to decrease if the clouds or precipitation are moving...
5.0K
Conservation of Angular Momentum: Application
12.4K
A system's total angular momentum remains constant if the net external torque acting on the system is zero. Examples of such systems include a freely spinning bicycle tire that slows over time due to torque arising from friction, or the slowing of Earth's rotation over millions of years due to frictional forces exerted on tidal deformations. However in the absence of a net external torque, the angular momentum remains conserved. The conservation of angular momentum principle requires a...
12.4K
Detection of Black Holes
2.6K
Although black holes were theoretically postulated in the 1920s, they remained outside the domain of observational astronomy until the 1970s.
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
2.6K
Schwarzschild Radius and Event Horizon
2.9K
No object with a finite mass can travel faster than the speed of light in a vacuum. This fact has an interesting consequence in the domain of extremely high gravitational fields.
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape...
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape...
2.9K
Doppler Effect - I
6.8K
The Doppler effect and Doppler shift were named after the Austrian physicist and mathematician Christian Johann Doppler in 1842, who conducted experiments with both moving sources and moving observers. Consider an observer standing on a street corner, observing an ambulance with a siren sound passing by at a constant speed. The observer experiences two characteristic changes in the sound of the siren. Initially, the sound increases in loudness as the ambulance approaches and decreases in...
6.8K
Atomic Nuclei: Larmor Precession Frequency
3.4K
The earth's gravitational field produces a 'twisting force' perpendicular to the angular momentum of a spinning mass (such as a spinning top) that causes the mass to 'wobble' around the gravitational field axis in a phenomenon called precession. Similarly, the magnetic moment (μ) of a spinning nucleus precesses due to an external magnetic field directed along the z-axis. The precession of the magnetic moment vector about the magnetic field is called Larmor precession,...
3.4K

