检测引力透镜放大Ia型超新星的探测
Robert M Quimby1, Masamune Oguri, Anupreeta More
1Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, The University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa-shi, Chiba 277-8583, Japan.
概括
天文学家证实了一颗Ia型超新星 (SNIa) 被前景星系放大.
科学领域:
- 宇宙学的宇宙学是什么?
- 天体物理学 天体物理学
- 引力透镜是一种引力透镜.
背景情况:
- 一类超新星 (SNIa) 对于测量宇宙距离至关重要.
- 大质量物体的引力透镜可以创建SNIa的多个图像,使宇宙膨胀的测试成为可能.
- 从其他现象中区分透镜SNIa是一个挑战.
研究的目的:
- 解决关于明亮超新星的争论:一种新型或放大SNIa.
- 确认SNIa被前景星系强烈放大的第一个例子.
- 探索发现更多透镜SNIa.Ia的方法.
主要方法:
- 在超新星的光线消失后获得了超新星的光谱.
- 分析了光谱,以确定前景星系的存在.
- 将观测数据与对透镜超新星的预测进行了比较.
主要成果:
- 证实超新星是Ia型超新星 (SNIa),由前景星系强烈放大.
- 衰光后的光谱揭示了透镜星系,解决了观测辩论.
- 这些发现表明,可能存在比以前估计的更多的透镜SNIa.
结论:
- 这项研究是首次证实SNIa被前景星系强烈引力放大的案例.
- 这一发现证实了SNIa在强透镜系统中作为探针的使用.
- 未来的调查可能会产生比预期的更高的SNIa发现率.
相关概念视频
Detection of Black Holes
1.7K
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...
1.7K
Schwarzschild Radius and Event Horizon
2.2K
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...
2.2K
Newton's Law of Gravitation
11.8K
Our everyday observation tells us that all objects close to the Earth naturally tend to fall to the ground. Early philosophers assumed that this downward force was unique to Earth. By the 16th century, Nicolaus Copernicus (1473-1543) put forward the heliocentric theory, which suggested that Earth and other planets orbited the sun, while the Moon orbited the Earth. However, it was Isaac Newton (1642-1727) who linked these two motions together in the 17th century. He reasoned that the force of...
11.8K
Doppler Effect - II
4.2K
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...
4.2K
Doppler Effect - I
4.7K
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...
4.7K
The Principle of Superposition and the Gravitational Field
2.3K
The principle of superposition applies to gravitational forces of objects that are sufficiently far apart. It states that the net gravitational force on a point object is the vector sum of the gravitational forces on it due to various objects. The principle helps calculate the force by listing the individual forces and then vectorially summing them up. However, it should be noted that the principle of superposition is not always apparent. In the presence of a second force, the first force could...
2.3K


