宇宙中第一个恒星的形成
Tom Abel1, Greg L Bryan, Michael L Norman
1Harvard Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA.
概括
模拟显示,每颗银河系前光环中只有一个大质量,无金属的恒星形成. 这发生在气体冷却和崩时,形成密集的核心,迅速收缩成单一的原星,限制了进一步的恒星形成.
科学领域:
- 宇宙学的宇宙学是什么?
- 天体物理学 天体物理学
- 计算科学 计算科学
背景情况:
- 结构形成模型表明,黑暗物质最初占主导地位,星系前物体是由密度扰动形成的.
- 原始气体通过分子冷却,沉入暗物质潜在井,形成分子云类型.
研究的目的:
- 模拟宇宙中第一个恒星之一的形成,使用自相一致的3D水力动力模型.
- 研究早期宇宙结构中的碎片化和恒星形成过程.
主要方法:
- 采用了一个完全自相一致的三维水力动力学模拟.
- 该模拟追踪了暗物质光环中的原始气体的崩,包括冷却和分子形成.
主要成果:
- 一个大约100太阳质量的密集核心形成并经历了快速收缩.
- 与预期相反,核心没有分裂;相反,一个单一的1太阳质量原星通过三体H2形成形成.
- 观察到快速积累 (每年10^-2太阳质量) 和原恒星的辐射反.
结论:
- 每个银河系前光环最多会形成一颗大质量,无金属的恒星.
- 来自形成恒星的辐射反抑制了同一个光环内的进一步恒星形成.
- 结果与银河系光环中金属贫富恒星的丰富度测量一致.
相关概念视频
Conditions on Early Earth
Around 4 billion years ago, oceans began to condense on earth while volcanic eruptions released nitrogen, carbon dioxide, methane, ammonia, and hydrogen into the primordial atmosphere. However, organisms with the characteristics of life were not initially present on earth. Scientists have used experimentation to determine how organisms evolved that could grow, reproduce, and maintain an internal environment.
Conditions on Early Earth
Around 4 billion years ago, oceans began to condense on earth while volcanic eruptions released nitrogen, carbon dioxide, methane, ammonia, and hydrogen into the primordial atmosphere. However, organisms with the characteristics of life were not initially present on earth. Scientists have used experimentation to determine how organisms evolved that could grow, reproduce, and maintain an internal environment.
Kepler's First Law of Planetary Motion
In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. He formulated his first two laws based on the observations of his forebears, Nikolaus Copernicus and Tycho Brahe.
Polish astronomer Nikolaus Copernicus put forth a theory that stated a heliocentric model for the solar system. According to this heliocentric theory, all the planets, including Earth, orbit the Sun in circular orbits.
On the other hand,...
Polish astronomer Nikolaus Copernicus put forth a theory that stated a heliocentric model for the solar system. According to this heliocentric theory, all the planets, including Earth, orbit the Sun in circular orbits.
On the other hand,...
Schwarzschild Radius and Event Horizon
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 velocity with the...
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 velocity with the...
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...
Space-Time Curvature and the General Theory of Relativity
In 1905, Albert Einstein published his special theory of relativity. According to this theory, no matter in the universe can attain a speed greater than the speed of light in a vacuum, which thus serves as the speed limit of the universe.
This has been verified in many experiments. However, space and time are no longer absolute. Two observers moving relative to one another do not agree on the length of objects or the passage of time. The mechanics of objects based on Newton's laws of motion,...
This has been verified in many experiments. However, space and time are no longer absolute. Two observers moving relative to one another do not agree on the length of objects or the passage of time. The mechanics of objects based on Newton's laws of motion,...


