罗氏叶性质的计算器

Denis A Leahy, Janet C Leahy
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引用次数: 10

摘要

罗氏波瓣几何对于理解和研究半分离二元体系中质量损失分量的性质是很重要的。然而,精确计算并不容易,现有的表通常不包括所研究的双星系统的参数,也不允许非同步旋转。罗氏叶的性质的计算器提出了两种格式。一个易于使用的Java版本有一个图形界面,而Fortran 90版本有一个命令行界面。Fortran版本允许用户轻松修改。两个版本都有两个基本输出选项:一个提供一组不同数量的值(例如沿二轴的拉格朗日点,以及罗氏叶的面积和体积);第二个提供\(R(\theta,\phi)\),在任何指定的极角下,从恒星中心到恒星表面的距离。可以直接输入单个输入参数集,也可以在文本文件中指定大量输入参数集。计算器包括选择有非同步旋转的星,或有星下填充其罗氏瓣。它可以用来计算椭圆轨道的罗氏叶性质,但有一些限制。我们提供了一个方便的软件工具,可以快速准确地计算质量比在0.01 ~ 100范围内的罗氏叶特性,罗氏叶填充因子在0.1 ~ 1.0范围内,以及恒星的无因次旋转速率在0.1 ~ 2.0范围内。这将允许任何研究双星系统的人获得他们系统的罗氏叶或恒星表面几何形状。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

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A calculator for Roche lobe properties

The Roche lobe geometry is important to understand and study the properties of the mass-losing component in a semi-detached binary system. However it is not easy to calculate accurately, and existing tables usually do not include the parameters of the binary system under study, nor do they allow for non-synchronous rotation.

A calculator for properties of the Roche lobe is presented in two formats. An easy-to-use Java version has a graphic interface, and a Fortran 90 version has a command line interface. The Fortran version allows for easy modifications by the user. Both versions have two basic output options: one provides values of a set of various quantities (such as the Lagrange points along the binary axis, and area and volume of the Roche lobe); the second provides \(R(\theta,\phi)\), the distance from the stellar center to the stellar surface for any specified polar angle. A single set of input parameters can be entered directly or a large set of input parameters can be specified in a text file. The calculator includes the options to have non-synchronous rotation of the star, or to have the star underfill its Roche lobe. It can be used to calculate Roche lobe properties for the case of elliptical orbits, with some restrictions.

We present a convenient software tool for quickly and accurately calculating Roche lobe properties for mass ratio in the range 0.01 to 100, for Roche lobe fill-out factor in the range 0.1 to 1.0, and for dimensionless rotation rate of the star in the range 0.1 to 2.0. This will allow anyone working with a binary star system to obtain the Roche lobe or stellar surface geometry for their system.

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期刊介绍: Computational Astrophysics and Cosmology (CompAC) is now closed and no longer accepting submissions. However, we would like to assure you that Springer will maintain an archive of all articles published in CompAC, ensuring their accessibility through SpringerLink's comprehensive search functionality.
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