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相关概念视频

Emission Spectra02:39

Emission Spectra

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.
Atomic Nuclei: Larmor Precession Frequency01:11

Atomic Nuclei: Larmor Precession Frequency

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, and the angular frequency...
IR Frequency Region: X–H Stretching01:24

IR Frequency Region: X–H Stretching

In IR spectroscopy, signals produced by the X−H bonds (such as C−H, O−H, or N−H) can be observed in the frequency range of  2700–4000 cm–1. The C−H stretching vibration forms sharp bands in the region 2850–3000 cm–1. The presence of the O−H stretching vibration leads to the forming of an absorption band in the frequency range 3650–3200 cm−1. At the same time, N−H stretching can be confirmed by absorption bands in the 3500–3100 cm−1 range. Even though both O−H and N−H bonds vibrate at a similar...
Atomic Absorption Spectroscopy: Radiation and Light Sources01:13

Atomic Absorption Spectroscopy: Radiation and Light Sources

Atomic absorption spectroscopy (AAS) relies on the Beer-Lambert law, which requires that the radiation source emits a narrow range of wavelengths to match the absorption characteristics of the analyte atom. The primary criteria for choosing an appropriate radiation source in AAS is to provide a precise and intense emission at specific wavelengths that will allow accurate detection of the analyte.
Two common narrow-range 'line' sources used in AAS are hollow-cathode lamps (HCLs) and...
Atomic Emission Spectroscopy: Overview01:20

Atomic Emission Spectroscopy: Overview

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...
Atomic Emission Spectroscopy: Instrumentation01:22

Atomic Emission Spectroscopy: Instrumentation

The instrumentation of atomic emission spectrometry (AES) involves various components, including atomization devices that convert samples into gas-phase atoms and ions. There are two main types of atomization devices: continuous and discrete atomizers.  Continuous atomizers, like plasmas and flames, introduce samples in a constant stream, while discrete atomizers inject individual samples using syringes or autosamplers. The most common discrete atomizer is the electrothermal atomizer.

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相关实验视频

Updated: Jul 6, 2026

The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry
12:14

The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry

Published on: August 12, 2013

在M82中超发光X射线源的轨道周期.

Philip Kaaret1, Melanie G Simet, Cornelia C Lang

  • 1Department of Physics and Astronomy, University of Iowa, Van Allen Hall, Iowa City, IA 52242, USA. philip-kaaret@uiowa.edu

Science (New York, N.Y.)
|January 10, 2006
PubMed
概括
此摘要是机器生成的。

银河系M82中的超发光X射线源 (ULX) 可能是一个中等质量的黑洞. 它的62天轨道周期表明它是一个巨星捐赠者,这表明它处于一个短暂的进化阶段.

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Characterizing Far-infrared Laser Emissions and the Measurement of Their Frequencies
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Characterizing Far-infrared Laser Emissions and the Measurement of Their Frequencies

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11:21

Cooling an Optically Trapped Ultracold Fermi Gas by Periodical Driving

Published on: March 30, 2017

相关实验视频

Last Updated: Jul 6, 2026

The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry
12:14

The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry

Published on: August 12, 2013

Characterizing Far-infrared Laser Emissions and the Measurement of Their Frequencies
09:38

Characterizing Far-infrared Laser Emissions and the Measurement of Their Frequencies

Published on: December 18, 2015

Cooling an Optically Trapped Ultracold Fermi Gas by Periodical Driving
11:21

Cooling an Optically Trapped Ultracold Fermi Gas by Periodical Driving

Published on: March 30, 2017

科学领域:

  • * 天体物理学 * 天体物理学
  • * 天文学 * 天文学
  • *X射线天文学 *X射线天文学

背景情况:

  • *超发光X射线源 (ULX) 是点状的X射线源,其发光度超过了恒星质量黑洞的爱丁顿极限.
  • *银河系M82拥有一个突出的ULX,这是一个中等质量黑洞 (IMBH) 的潜在候选者.
  • *超级星团是强烈恒星形成和动态相互作用的场所,可能导致IMBH形成.

研究的目的:

  • * 为了研究M82.2.中的ULX的性质.
  • * 确定ULX二进制星系的轨道周期和特征.
  • * 为了限制紧物体及其伴侣的质量和进化状态.

主要方法:

  • *分析从M82.2.的X射线流量调制.
  • * 确定X射线辐射的周期性.
  • * 在二进制进化的背景下对轨道周期的解释.

主要成果:

  • * 来自M82 ULX的X射线流表现出显著的调制.
  • *确定了62.0±2.5天的周期,解释为轨道周期.
  • *推断的轨道周期表明质量捐赠恒星是一个巨星或超级巨星.

结论:

  • *M82 ULX可能是一个X射线双星系统,有一个中等质量的黑洞.
  • *伴星处于巨型阶段,体验着高质量转移率.
  • * 观测到的ULX代表了二进制星进化的短暂而不寻常的阶段.