最年轻的恒星的外流大多是分子的
T P Ray1,2, M J McCaughrean3, A Caratti O Garatti4
1Dublin Institute for Advanced Studies, Dublin, Ireland. tr@cp.dias.ie.
Nature
|August 24, 2023
概括
年轻的恒星通过强大的喷气驱逐物质. 新的詹姆斯·韦伯太空望远镜的观测显示这些喷射主要由热分子组成,而不是原子或离子,
科学领域:
- * 天体物理学
- * 恒星形成
- * 星球科学
背景情况:
- * 恒星和行星的形成包括通过超音速喷气的物质积聚和驱逐.
- * 年轻的原星表现出最强大的喷气, 但被尘埃遮蔽, 限制了观测.
- 形成喷气背骨的热,原子,离子和分子组成部分在很大程度上没有被观察到.
研究的目的:
- * 调查年轻的原星喷气的组成,特别是它们的热成分.
- 为了解释原恒星外流中观察到的"绿色模糊"的起源.
- * 通过红外观测探测喷气演变的早期阶段.
主要方法:
- *使用詹姆斯·韦伯太空望远镜 (JWST) 进行近红外观测.
- * 针对 Herbig-Haro 211 的定位观测,这是一个年轻的原星的外流.
- *分析热分子,原子和离子气体的辐射.
主要成果:
- * 在Herbig-Haro 211外流中检测到大量的热分子排放.
- 这些"绿色模糊"被解释为这些热分子的辐射.
- * 喷射脊柱几乎纯粹是分子,原子或离子辐射最小.
- * 与更发达的喷气相比,外流的传播速度较慢.
结论:
- * 年轻的原恒星喷流的骨干主要是分子.
- *JWST的红外能力对于观察原恒星外流的隐蔽,热组件至关重要.
- 这项研究为喷气形成和进化的早期阶段提供了新的见解.
相关概念视频
Distribution of Molecular Speeds
4.0K
The motion of molecules in a gas is random in magnitude and direction for individual molecules, but a gas of many molecules has a predictable distribution of molecular speeds. This predictable distribution of molecular speeds is known as the Maxwell-Boltzmann distribution. The distribution of molecular speeds in liquids is comparable to that of gases but not identical and can help to understand the phenomenon of the boiling and vapor pressure of a liquid. Consider that a molecule requires a...
4.0K
Atomic Emission Spectroscopy: Overview
2.3K
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...
2.3K
Emission Spectra
54.3K
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.
54.3K
Atomic Emission Spectroscopy: Lab
197
AES is a powerful analytical technique, especially effective when used with plasma sources, producing abundant spectra in characteristic emission lines. The Inductively Coupled Plasma (ICP), in particular, yields superior quantitative analytical data due to its high stability, low noise, low background, and minimal interferences under optimal experimental conditions. However, newer air-operated microwave sources are emerging as promising alternatives that could be more cost-effective than...
197
Molecular Kinetic Energy
5.1K
The word "gas" comes from the Flemish word meaning "chaos," first used to describe vapors by the chemist J. B. van Helmont. Consider a container filled with gas, with a continuous and random motion of molecules. During collisions, the velocity component parallel to the wall is unchanged, and the component perpendicular to the wall reverses direction but does not change in magnitude. If the molecule’s velocity changes in the x-direction, then its momentum is changed.
5.1K
Behavior of Gas Molecules: Molecular Diffusion, Mean Free Path, and Effusion
29.1K
Although gaseous molecules travel at tremendous speeds (hundreds of meters per second), they collide with other gaseous molecules and travel in many different directions before reaching the desired target. At room temperature, a gaseous molecule will experience billions of collisions per second. The mean free path is the average distance a molecule travels between collisions. The mean free path increases with decreasing pressure; in general, the mean free path for a gaseous molecule will be...
29.1K


