一个强烈的紫外线脉冲来自一个新生的类型Ia超新星
Yi Cao1, S R Kulkarni2, D Andrew Howell3
1Astronomy Department, California Institute of Technology, Pasadena, California 91125, USA.
Nature
|May 22, 2015
概括
观测显示,来自Ia型超新星的强紫外线辐射,为单一退化的祖先通道提供了证据. 这一发现有助于解释这些宇宙爆炸的起源及其用于测量宇宙距离的用途.
科学领域:
- 天文学和天体物理学
- 宇宙学的宇宙学是什么?
背景情况:
- 类型Ia超新星对于测量宇宙学距离至关重要.
- 它们的祖先的确切性质,特别是白矮星系统,仍然是活跃的研究领域.
- 单一退化通道模型提出一个白矮星从伴星中增加物质.
研究的目的:
- 为了研究Ia型超新星的原始系统.
- 收集支持或反驳单一退化通道模型的观察证据.
主要方法:
- 使用Swift太空望远镜进行观测.
- 分析来自Ia型超新星在爆炸后四天内发出的紫外线辐射数据.
主要成果:
- 在超新星事件发生后不久检测出强烈的,下降的紫外线辐射.
- 观测到的发射模式与射出伴星相互作用的理论预测一致.
结论:
- 这些发现为单一退化通道作为一些Ia型超新星的祖先途径提供了令人信服的观测证据.
- 这支持使用Ia型超新星作为宇宙学中的标准.
相关概念视频
Ultraviolet and Visible (UV–Vis) Spectroscopy: Overview
8.6K
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...
8.6K
Emission Spectra
79.1K
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.
79.1K
NMR Spectrometers: Radiofrequency Pulses and Pulse Sequences
2.1K
A pulse is a short burst of radio waves distributed over a range of frequencies that simultaneously excites all the nuclei in the sample. Upon passing a radio frequency pulse along the x-axis, the nuclei absorb energy corresponding to their Larmor frequencies and achieve resonance. This shifts the net magnetization vector from the z-axis toward the transverse plane. This angle of rotation of the magnetization vector, or the flip angle, is proportional to the duration and intensity of the pulse.
2.1K
Atomic Emission Spectroscopy: Overview
4.4K
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...
4.4K
Infrared (IR) Spectroscopy: Overview
7.5K
When electromagnetic radiation passes through a material, atoms or molecules transition from a lower to a higher energy state by absorbing radiation corresponding to the energy difference between the two states. The absorption of infrared (IR) radiation causes transitions between vibrational energy levels in a molecule. Therefore, IR spectroscopy is a useful analytical tool for determining the molecular structure of molecules.
Different compounds display unique properties due to their...
Different compounds display unique properties due to their...
7.5K
Nuclear Fusion
35.4K
The process of converting very light nuclei into heavier nuclei is also accompanied by the conversion of mass into large amounts of energy, a process called fusion. The principal source of energy in the sun is a net fusion reaction in which four hydrogen nuclei fuse and ultimately produce one helium nucleus and two positrons.
A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...
A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...
35.4K


