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相关概念视频

Emission Spectra02:39

Emission Spectra

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When solids, liquids, or condensed gases are heated sufficiently, they radiate some of the excess energy as light. Photons produced in this manner have a range of energies, and thereby produce a continuous spectrum in which an unbroken series of wavelengths is present.
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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...
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Ultraviolet and Visible (UV–Vis) Spectroscopy: Overview01:02

Ultraviolet and Visible (UV–Vis) Spectroscopy: Overview

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Ultraviolet–visible (UV–visible or UV–Vis) spectroscopy is an analytical technique that investigates the interaction between matter and UV–Vis light within the electromagnetic spectrum. This method is widely used for its versatility, simplicity, and relatively quick data acquisition, making it valuable for both qualitative and quantitative analysis. When UV–Vis radiation passes through a material,  molecules absorb light depending on the energy required for...
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Atomic Emission Spectroscopy: Overview01:20

Atomic Emission Spectroscopy: Overview

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Atomic emission spectroscopy (AES) is an analytical technique used to determine the elemental composition of a sample by analyzing the light emitted from excited atoms. In AES, atoms in a sample are excited to higher energy levels by thermal energy from high-temperature sources, such as plasma, arcs, or sparks. When these excited atoms return to lower energy states, they emit light at specific wavelengths characteristic of each element. The resulting atomic emission spectrum, which consists of...
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Schwarzschild Radius and Event Horizon01:21

Schwarzschild Radius and Event Horizon

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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...
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Interaction of EM Radiation with Matter: Spectroscopy01:12

Interaction of EM Radiation with Matter: Spectroscopy

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Electromagnetic (EM) radiation can be considered an oscillating electric and magnetic field propagating through a medium that can interact with matter in its path. The electric field in the radiation can interact with electrical charges in the atoms or molecules in the matter. On the other hand, the magnetic field can interact with the magnetic field in the atomic nucleus. The study of the interaction between electromagnetic radiation and matter is termed spectroscopy. Spectroscopy is the study...
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相关实验视频

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Characterizing Far-infrared Laser Emissions and the Measurement of Their Frequencies
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在遥远的矮星系中扩展远紫外辐射

Anshuman Borgohain1, Kanak Saha2, Bruce Elmegreen3

  • 1Department of Physics, Tezpur University, Napaam, India. ayush.borgohain@gmail.com.

Nature
|July 21, 2022
PubMed
概括

我们使用AstroSat望远镜观察蓝矮星系的恒星形成. 这表明它们的外部区域正在发生气体积聚和引力不稳定.

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Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
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科学领域:

  • 天文学与天体物理学
  • 星系的形成和演变

背景情况:

  • 蓝色紧矮星系 (BCD) 的亮度低,金属缺乏,并且集中在中心,具有恒星形成团.
  • 观察BCD形成是具有挑战性的,因为在高红移时的模糊和小尺寸.
  • 中间红移观测对于研究BCD的早期进化阶段至关重要,特别是受气体积累影响的外部区域.

研究的目的:

  • 研究蓝矮星系的形成过程.
  • 分析BCD的外部区域中的恒星形成活动.

主要方法:

  • 使用阿斯特罗卫星上的紫外线成像望远镜观测GOODS南方领域的11个BCD.
  • 分析远紫外线 (FUV) 辐射,并与哈勃太空望远镜的光学数据进行比较.
  • 对仪表点扩散函数进行校正,以确定内在的FUV辐射轮.

主要成果:

  • 在0.1-0.24红移的11个BCD的外部区域检测到过度的紫外线 (FUV) 辐射.
  • 对于十个BCD,内在FUV发射的辐射形状显示出比光学对应的尺度长度更大.
  • 凸起的FUV结构表明外盘的引力不稳定性.

结论:

  • 浅浅的FUV形状表明宇宙积聚盘中的恒星形成有所扩大.
  • 外部FUV磁盘的引力不稳定性通过动态摩擦驱动团块向内移动.
  • 由于气体积聚和内部动态, BCD 外部区域正在积极演变.