首页> 外文OA文献 >Fourier analysis of unequally-spaced time series : with applications to the study of helium stars and binary systems
【2h】

Fourier analysis of unequally-spaced time series : with applications to the study of helium stars and binary systems

机译:等距时间序列的傅立叶分析:在氦恒星和双星系统研究中的应用

代理获取
本网站仅为用户提供外文OA文献查询和代理获取服务,本网站没有原文。下单后我们将采用程序或人工为您竭诚获取高质量的原文,但由于OA文献来源多样且变更频繁,仍可能出现获取不到、文献不完整或与标题不符等情况,如果获取不到我们将提供退款服务。请知悉。

摘要

The application of the discrete Fourier transform to the determination of the frequency content of unevenly-sampled astronomical time series is discussed, and an interactive computer package which incorporates a variety of power-spectrum and time-domain techniques is described.ududA frequency analysis of the light curves of two hot, extreme helium stars, BD-9°4395 and HD160641, shows that their photometric variability is caused by non-radial pulsation. Spectroscopic evidence in support of non-uniform mass loss is presented for BD-9°4395.ududSpectroscopic and photometric observations of two early-type eclipsing binary systems, AL Sculptoris and DM Persei, have been analysed to yield their absolute dimensions. AL Scl is found to be a detached system in which both components rotate faster than synchronism. The origin of distortions in its light curve is unclear. DH Per is shown to be part of a triple system in which the third component is most probably a late-B star in a 98-day orbit with a semi-major axis of 0.9 A.U. The binary system is confirmed to be semi-detached and to have evolved through a phase of rapid mass transfer. DH Per joins a small group of massive, semi-detached systems whose characteristics differ significantly from the classical Algols, and which may result from case-A, mass-transfer processes.ududSpectroscopic and photometric observations of the F4V star HD123058 do not support the hypothesis that it is a binary system. Broad lines in its spectrum are attributed to a somewhat enhanced rotation rate, and the star is shown to be essentially unevolved. The derivation of the equation of condition in Sterne's rigorousudmethod for the analysis of the spectroscopic elements of binary systems, and its modification for incorporating observed times of minimum light into the adjustment of the elements, are outlined. A computer code for the determination of orbital elements according to this scheme is described.
机译:讨论了离散傅里叶变换在确定采样不均匀的天文时间序列频率内容中的应用,并描述了一种交互式计算机软件包,该软件包结合了多种功率谱和时域技术。对两个高温的极端氦星BD-9°4395和HD160641的光曲线的分析表明,它们的光度变异性是由非辐射脉动引起的。 BD-9°4395提供了支持非均匀质量损失的光谱学证据。 ud ud分析了两个早期类型的日蚀双星系统AL Sculptoris和DM Persei的光谱学和光度学观测,以得出其绝对尺寸。发现AL Scl是一个独立的系统,其中两个组件的旋转速度都比同步速度快。其光曲线失真的原因尚不清楚。 DH Per被证明是三重系统的一部分,其中第三部分很可能是98天轨道上的B晚星,半长轴为0.9A.U。已确认该二元体系是半分离的,并且已经通过快速质量转移阶段进行了进化。 DH Per加入了一小组庞大的,半独立的系统,这些系统的特征与经典的算法明显不同,并且可能是由案例A的传质过程造成的。 ud udF4V星HD123058的光谱和光度观测支持这是一个二进制系统的假设。其光谱中的宽线归因于自转速度的提高,并且该恒星显示为基本未旋转。概述了Sterne严格的 udmethod中用于分析二元系统的光谱元素的条件方程的推导,以及将观察到的最小光时间纳入元素调整中的修改。描述了用于根据该方案确定轨道元素的计算机代码。

著录项

  • 作者

    Skillen W. J. I. (Ian);

  • 作者单位
  • 年度 1986
  • 总页数
  • 原文格式 PDF
  • 正文语种 en
  • 中图分类

相似文献

  • 外文文献
  • 中文文献
  • 专利

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号