点源在稠密环境中超音速运动的BONDI-HOYLE吸积尾

IF 1.1 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Revista Mexicana de Astronomia y Astrofisica Pub Date : 2022-10-01 DOI:10.22201/ia.01851101p.2022.58.02.04
A. Raga, J. Cantó, A. Castellanos-Ramírez, A. Rodríguez-González, P. Rivera-Ortiz
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引用次数: 0

摘要

我们提出了一个“Bondi Hoyle尾巴”的模型,该模型是由一个紧凑、大质量的物体通过密集、辐射环境的高超音速通道留下的。我们推导了沿尾部的流速和质量的简单方程,并获得了稳态问题的数值解和近似解析解。然后,我们研究了一个与时间相关的问题,在这个问题中,源首先在稠密的云中传播,然后出现在低密度的环境中。这种流动导致了致密气体的踪迹,在它从致密云中出现的地方与源相连。该轨迹的速度与位置呈线性关系。
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THE BONDI-HOYLE ACCRETION TAIL OF POINT SOURCES TRAVELLING HYPERSONICALLY THROUGH A DENSE ENVIRONMENT
We present a model for the “Bondi-Hoyle tail” left behind by the hypersonic passage of a compact, massive object through a dense, radiative environment. We derive simple equations for the flow velocity and the mass along the tail, and obtain numerical and approximate analytical solutions for the steady state problem. We then study a time-dependent problem in which the source first travels within a dense cloud, and then emerges into a low density environment. This flow results in the production of a trail of dense gas joining the source at the point in which it emerged from the dense cloud. This trail has a linear velocity vs. position profile.
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来源期刊
Revista Mexicana de Astronomia y Astrofisica
Revista Mexicana de Astronomia y Astrofisica 地学天文-天文与天体物理
CiteScore
1.30
自引率
10.00%
发文量
14
审稿时长
>12 weeks
期刊介绍: The Revista Mexicana de Astronomía y Astrofísica, founded in 1974, publishes original research papers in all branches of astronomy, astrophysics and closely related fields. Two numbers per year are issued and are distributed free of charge to all institutions engaged in the fields covered by the RMxAA.
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