相关实验视频
Updated: Jul 6, 2026

10:35
Bringing the Visible Universe into Focus with Robo-AO
Published on: February 12, 2013
激光导向恒星自适应光学成像极度测量赫尔比格Ae/Be恒星的极度测量
Marshall D Perrin1, James R Graham, Paul Kalas
1Astronomy Department, University of California Berkeley, Berkeley, CA 94720, USA. mperrin@astro.berkeley.edu
概括
我们使用先进的光学研究年轻恒星,揭示了极化星云和射流. 这表明T Tauri和Herbig Ae/Be恒星有着共同的进化路径.
科学领域:
- 天文学和天体物理学
- 恒星进化 恒星进化
- 环恒星环境 环恒星环境
背景情况:
- 赫尔比克Ae/Be恒星是中等质量的年轻恒星,对于理解恒星进化至关重要.
- 环恒星盘和外在恒星形成和行星系统发展中发挥着关键作用.
研究的目的:
- 通过先进的观测技术,研究赫尔比格Ae/Be恒星的环恒星环境.
- 为了比较中等质量的Herbig Ae/Be恒星与较低质量的T Tauri恒星的进化阶段.
主要方法:
- 利用激光导向星适应光学用于高分辨率成像.
- 采用近红外双通道成像极相仪来分析散射光.
主要成果:
- 在LkHalpha 198. 周围观测到一个极化强的双圆形星云.
- 检测到与嵌入式源LkHalpha 198-IR.相关的极化喷气式特征.
- 在LkHalpha 233中发现了一条狭窄的,未极化的黑暗轨道,表明有一个环恒星盘.
结论:
- 在Herbig Ae/Be恒星中观察到的特征与在较低质量的T Tauri恒星中观察到的过程是一致的.
- 这些发现支持T Tauri和Herbig Ae/Be星的共同进化序列.
相关概念视频
Detection of Black Holes
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...
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...
Two common narrow-range 'line' sources used in AAS are hollow-cathode lamps (HCLs) and...
Inductively Coupled Plasma Atomic Emission Spectroscopy: Instrumentation
Inductively coupled plasma (ICP) is the common plasma source used in atomic emission spectroscopy (AES), a technique that detects and analyzes various elements in a sample. This method is often called inductively coupled plasma atomic emission spectroscopy (ICP-AES).
There are three main types of inductively coupled plasma atomic emission spectroscopy (ICP-AES) instruments: sequential, simultaneous multichannel, and Fourier transform instruments, with the latter being less commonly used.
There are three main types of inductively coupled plasma atomic emission spectroscopy (ICP-AES) instruments: sequential, simultaneous multichannel, and Fourier transform instruments, with the latter being less commonly used.
Flame Photometry: Overview
Flame photometry, also known as flame emission spectrometry, is a technique used for the qualitative and quantitative analysis of elements present in a sample using a flame as the source of excitation energy. The concept of flame photometry was realized in the early 1860s by Kirchhoff and Bunsen, who discovered that specific elements emit characteristic radiation when excited in flames. The first instrument developed for this purpose was used to measure sodium (Na) in plant ash using a Bunsen...
Flame Photometry: Lab
In a flame photometer, when a solution like potassium chloride is aspirated into the flame, the solvent evaporates, leaving behind dehydrated salt. This salt dissociates into free gaseous atoms in their ground state. Some of these atoms absorb energy from the flame, leading to their excitation. The excited atoms return to the ground state, emitting photons at characteristic wavelengths. Because only electronic transitions are involved, the resulting emission lines are very narrow. The intensity...

